Notes/Physics/Paper 1/Physical Quantities and Units
CAIEAS Level9702§1.1–1.4

Physical Quantities and Units

Number and unit; SI base and derived units; prefixes; checking equations with units; systematic and random errors; combining uncertainties; scalars, vectors and components.

240 min read 8 sub-topics
271
question parts
2021–2025 · 37 papers
9 marks
per paper
≈ 9% of the paper
1.8/3
avg difficulty
moderate
#9
most examined
of 11 topics by marks

From O Level or IGCSE you already know that a measurement is a number with a unit, and that units such as the newton and the joule come from formulas like F=maF = ma. This first AS note makes those ideas exact and gives you tools that every later topic uses.

You start with what a physical quantity is and how to estimate one. Then you meet the SI base units, build other units from them, use prefixes such as milli and mega, and use units to check an equation. Next come measurement errors and how to combine uncertainties. Last, you add, subtract and split quantities that have a direction.

Before you start you should be able to
  • Standard form and powers of ten: writing 0.000520.00052 as 5.2×10−45.2 \times 10^{-4} and back again

  • Practical use of a ruler, protractor, stopwatch and thermometer

  • sin⁡\sin, cos⁡\cos and tan⁡\tan on a right-angled triangle (opposite/hypotenuse, adjacent/hypotenuse, opposite/adjacent)

  • Pythagoras' theorem for a right-angled triangle, and the cosine rule a2=b2+c2−2bccos⁡Aa^2 = b^2 + c^2 - 2bc\cos A for any triangle

  • Rearranging simple equations, e.g. finding kk from F=kxF = kx

  • Everyday SI units: metres, kilograms, seconds

  • O Level / IGCSE formulas: weight W=mgW = mg, pressure p=F/Ap = F/A, density ρ=m/V\rho = m/V, F=maF = ma

By the end of this page you can
  • State that every physical quantity is a numerical magnitude with a unit, and make reasonable order-of-magnitude estimates of common quantities

  • Recall the five SI base quantities and their units, tell base quantities from derived ones, and express derived units (N, J, W, Pa, C, V…) as products/quotients of base units

  • Convert between prefixed units from pico (p) to tera (T), including squared and compound units

  • Use base units to check the homogeneity of an equation, find the base units of a constant, and find an unknown power

  • Distinguish systematic (including zero) errors from random errors, correct a zero error, and tell precision from accuracy

  • Assess the uncertainty in a derived quantity by combining absolute or percentage uncertainties, including powers, and decide whether two results agree

  • Classify quantities as scalars or vectors; add and subtract coplanar vectors by drawing or with the cosine rule, including a change in velocity

  • Resolve a vector into two perpendicular components, add vectors by components, and recombine components into a resultant

01

Physical quantities and estimates

Syllabus requirement · §1.1

“

understand that all physical quantities consist of a numerical magnitude and a unit; make reasonable estimates of physical quantities included within the syllabus

”

A number of what?

Physics is measurement, and every measurement answers the question "how much of what?". A physical quantity is therefore always two things stapled together: a numerical magnitude (how much) and a unit (of what). The distance to the nearest town is not "6.86.8" — it is 6.8 km6.8\ \text{km}. The current in a wire is not "0.500.50" — it is 0.50 A0.50\ \text{A}. Strip the unit away and the number stops meaning anything: 6.86.8 could be 6.8 km6.8\ \text{km}, 6.8 kg6.8\ \text{kg} or 6.8 N6.8\ \text{N}, and those are three completely different physical situations.

The unit is part of the answer

Every quantity in this course is a number of something. In an exam, a missing or wrong unit loses the mark exactly as a wrong number does — an answer of "6.86.8" to "find the force" is not 90% correct, it is meaningless. Later in this note (see “Checking equations with base units”) you will see that units also do real work: carried through an equation, they catch algebra mistakes before they reach your final answer.

Estimates: anchoring to what you know

Examiners frequently ask for an order-of-magnitude estimate of an everyday quantity — the weight of a person, the pressure of a person standing, the wavelength of ultraviolet light. Nobody memorises these answers. The skill being tested is whether you can anchor to a small set of reference values you do know, and build the wanted quantity from them.

Here are the anchors worth carrying into the exam:

Reference

Value to anchor to

Mass of an adult

≈ 70–80 kg

Height of an adult

≈ 1.7 m

Weight of an adult

≈ 700 N (from W=mgW = mg)

Acceleration of free fall

g=9.81 m s−2g = 9.81\ \text{m s}^{-2}

Area under one shoe sole

≈ 0.025 m²

Walking speed; a car on a motorway

≈ 1.5 m s⁻¹; ≈ 30 m s⁻¹

Power of an electric kettle

≈ 2000 W

Wavelength of visible light

≈ 4 × 10⁻⁷ m (violet) to 7 × 10⁻⁷ m (red)

Diameter of an atom

≈ 10⁻¹⁰ m

Note the third row: weight is a force, measured in newtons. A "weight of 70" for an adult is a category error — 70 is the mass in kg, and the classic trap in estimate questions.

Making an order-of-magnitude estimate
  1. 1

    Anchor to a reference value you know.

    Estimation questions are marked by range, not by an exact figure — an anchor you trust is worth more than a guess at precision.

  2. 2

    Build the wanted quantity from the anchor, using a defining equation where one exists (e.g. weight from W=mgW = mg, pressure from p=F/Ap = F/A).

  3. 3

    Give the answer as a power of ten (or to 1 significant figure) with the correct unit.

    An estimate without its unit is not an answer — and the unit often exposes the trap, as the next worked example shows.

A clean demonstration

Estimate, to the nearest power of ten, the weight of a school bag loaded with textbooks.

Step 1 — anchor. A hardback textbook has a mass of about 1.1 kg1.1\ \text{kg} (a phone is about 0.2 kg0.2\ \text{kg}; the book is five or more of those). An empty bag is about 0.5 kg0.5\ \text{kg}. So the loaded bag has

m≈0.5+(5×1.1)≈6 kgm \approx 0.5 + (5 \times 1.1) \approx 6\ \text{kg}

Step 2 — build the wanted quantity. Weight is a force, so it comes from W=mgW = mg. Here m=6 kgm = 6\ \text{kg} and g=9.81 m s−2g = 9.81\ \text{m s}^{-2}:

W=6×9.81=58.9 N≈59 NW = 6 \times 9.81 = 58.9\ \text{N} \approx 59\ \text{N}

Step 3 — give the answer as a power of ten. To one significant figure 59 N≈6×101 N59\ \text{N} \approx 6 \times 10^{1}\ \text{N}; as an order of magnitude (the nearest power of ten) it is 102 N10^{2}\ \text{N}. Either form, with its unit, is a complete estimate.

Estimating the weight of an adult

9702/12 O/N 2025 Q1

What is a reasonable estimate of the weight of an adult human?

Options

A   7×100 N7 \times 10^{0}\ \text{N}
B   7×102 N7 \times 10^{2}\ \text{N}
C   7×104 N7 \times 10^{4}\ \text{N}
D   7×106 N7 \times 10^{6}\ \text{N}

Show full working
  1. 1

    Read the unit off the options before any arithmetic: every answer is in newtons, N\text{N} — a force. Weight is a force, so the answer must come from a force equation; a bare mass in kilograms cannot be the answer.

    The classic trap here is answering 70 — the mass. Checking the unit first (N, not kg) rules that trap out immediately.

  2. 2

    Anchor the estimate: the mass of an adult is m≈70 kgm \approx 70\ \text{kg}.

    Anchoring is the whole skill: everything is built from a reference you already know.

  3. 3

    Weight comes from W=mgW = mg. Identify each piece the formula needs: m=70 kgm = 70\ \text{kg} and g=9.81 m s−2g = 9.81\ \text{m s}^{-2}, then substitute: W=70×9.81W = 70 \times 9.81

    Say what each symbol equals here before multiplying — this is the habit that stops mass and weight being confused.

  4. 4

    Evaluate: W=70×9.81=686.7 N≈690 NW = 70 \times 9.81 = 686.7\ \text{N} \approx 690\ \text{N}

  5. 5

    Express to one significant figure: 690 N≈7×102 N690\ \text{N} \approx 7 \times 10^{2}\ \text{N}. The options are spaced by factors of 100100, so only 7×102 N7 \times 10^{2}\ \text{N} is in the right ballpark — option B.

    690 N is 6.9×1026.9 \times 10^{2} N; the neighbouring options 7×1007 \times 10^{0} and 7×1047 \times 10^{4} are a hundred times too small and too large.

Answer

B — 7×102 N7 \times 10^{2}\ \text{N} (an adult of mass ≈ 70 kg has weight W=mg≈690 NW = mg \approx 690\ \text{N}).

Convert mass to weight with W=mgW = mg before comparing options — and read the options' unit first: if it is N, a mass answer cannot be right.

Your turn

The first checks the idea of a physical quantity. The rest are anchor → build → power of ten. If your answer's unit does not match the question's, stop and re-read.

  1. 19702/14 O/N 2025 Q1

    What is essential to accurately represent all physical quantities?

    Options

    A   a base unit and a number
    B   a unit and a number expressed in standard form (scientific notation)
    C   a unit and a numerical magnitude
    D   an SI unit and a numerical magnitude

    Show solution
    1. 1

      Recall the idea from the start of this section: every physical quantity is a numerical magnitude together with a unit. That is option C.

    2. 2

      A fails: the unit need not be a base unit (one of the five basic SI units in the next section). A force of 6.8 N6.8\ \text{N} is complete, and the newton is not a base unit.

      Each wrong option adds an extra condition. Look for the word that makes the condition too strict.

    3. 3

      B fails: standard form is a convenient way to write a number, but 6.8 km6.8\ \text{km} is a complete quantity without it.

    4. 4

      D fails: the unit need not be SI. A journey of 3 hours3\ \text{hours} or 20 miles20\ \text{miles} is still a physical quantity.

    Answer

    C — a unit and a numerical magnitude.

  2. 29702/13 O/N 2025 Q15

    A man of weight 600 N600\ \text{N} stands with both feet flat on the ground.

    What is a reasonable estimate of the pressure exerted on the ground by the weight of the man?

    Options

    A   1×100 Pa1 \times 10^{0}\ \text{Pa}
    B   1×102 Pa1 \times 10^{2}\ \text{Pa}
    C   1×104 Pa1 \times 10^{4}\ \text{Pa}
    D   1×106 Pa1 \times 10^{6}\ \text{Pa}

    Stuck? Show hint

    Estimate the total area of both shoe soles first — pressure is force per unit area.

    Show solution
    1. 1

      Pressure is force per unit area: p=FAp = \dfrac{F}{A}. Identify the pieces: the force is the man's weight, F=600 NF = 600\ \text{N} (already a force in newtons — no conversion needed), and AA is the total area in contact with the ground, i.e. both soles.

      Two things to get right before any arithmetic: the force is the weight in N, and the area is both feet together, not one.

    2. 2

      Anchor the area: one shoe sole is roughly a rectangle 25 cm×10 cm25\ \text{cm} \times 10\ \text{cm}, so Aone≈0.25×0.10=0.025 m2A_{\text{one}} \approx 0.25 \times 0.10 = 0.025\ \text{m}^2 Both feet: A≈2×0.025=0.05 m2A \approx 2 \times 0.025 = 0.05\ \text{m}^2

    3. 3

      Substitute into the defining equation: p=6000.05p = \frac{600}{0.05}

    4. 4

      Evaluate: p=6000.05=12 000 Pa=1.2×104 Pap = \frac{600}{0.05} = 12\,000\ \text{Pa} = 1.2 \times 10^{4}\ \text{Pa} — an order of magnitude of 104 Pa10^{4}\ \text{Pa}, option C.

      Dividing by 0.05 is the same as multiplying by 20: 600×20=12 000600 \times 20 = 12\,000.

    Answer

    C — 1×104 Pa1 \times 10^{4}\ \text{Pa} (p=600/0.05=1.2×104 Pap = 600 / 0.05 = 1.2 \times 10^{4}\ \text{Pa} for a total sole area of about 0.05 m20.05\ \text{m}^2).

  3. 39702/14 M/J 2025 Q1

    The number of atoms in a mobile phone handset may be estimated by dividing the approximate volume of the handset by the approximate volume of an atom.

    What is a reasonable estimate of the number of atoms in a mobile phone handset?

    Options

    A   101710^{17}
    B   102610^{26}
    C   103210^{32}
    D   103710^{37}

    Stuck? Show hint

    Work in metres throughout. An atom is about 10−10 m10^{-10}\ \text{m} across.

    Show solution
    1. 1

      Anchor the size of the phone: about 15 cm15\ \text{cm} long, 7 cm7\ \text{cm} wide and 1 cm1\ \text{cm} thick. Write these in metres straight away: 0.15 m0.15\ \text{m}, 0.07 m0.07\ \text{m} and 0.01 m0.01\ \text{m}.

      Both volumes must be in the same unit before you divide. Metres avoid any unit-conversion trap.

    2. 2

      Volume of the phone: Vphone≈0.15×0.07×0.01=1.05×10−4 m3≈10−4 m3V_{\text{phone}} \approx 0.15 \times 0.07 \times 0.01 = 1.05 \times 10^{-4}\ \text{m}^3 \approx 10^{-4}\ \text{m}^3

    3. 3

      Anchor the atom: its diameter is about 10−10 m10^{-10}\ \text{m}. Treat it as a small cube of that side, so Vatom≈(10−10)3=10−30 m3V_{\text{atom}} \approx (10^{-10})^3 = 10^{-30}\ \text{m}^3

      For an order of magnitude, a cube is close enough to a sphere. The cube gives the power: (10−10)3=10−30(10^{-10})^3 = 10^{-30}, not 10−1310^{-13}.

    4. 4

      Divide: N≈VphoneVatom=10−410−30N \approx \frac{V_{\text{phone}}}{V_{\text{atom}}} = \frac{10^{-4}}{10^{-30}}

    5. 5

      Subtract the powers: N≈10−4−(−30)=1026N \approx 10^{-4 - (-30)} = 10^{26} — option B.

    Answer

    B — about 102610^{26} atoms (10−4 m3÷10−30 m310^{-4}\ \text{m}^3 \div 10^{-30}\ \text{m}^3).

  4. 49702/21 O/N 2019 Q1(a)(i)

    Make an estimate of the mass, in g, of a new pencil.

    Stuck? Show hint

    Anchor to a small mass you know — a sheet of A4 paper has a mass of about 5 g.

    Show solution
    1. 1

      Anchor: a sheet of A4 paper has a mass of about 5 g5\ \text{g}. A pencil contains roughly a few sheets' worth of wood plus a thin graphite core, so its mass is a few grams.

      Estimation answers are marked by range, not by an exact value — the anchor gets you to the right order of magnitude, which is all that is required.

    2. 2

      A reasonable estimate is therefore about 55–10 g10\ \text{g}. The mark scheme accepts anywhere in the range 11–20 g20\ \text{g}.

      100100 g would be a small apple and 11 g a paperclip — the pencil sits between those neighbouring orders of magnitude.

    Answer

    Any value in the range 11–20 g20\ \text{g} (a typical new pencil is about 55–10 g10\ \text{g}).

  5. 5

    Which of the following is a reasonable estimate for the wavelength of ultraviolet radiation?

    Options

    A   1×10−15 m1 \times 10^{-15}\ \text{m}
    B   1×10−7 m1 \times 10^{-7}\ \text{m}
    C   1×10−3 m1 \times 10^{-3}\ \text{m}
    D   1×102 m1 \times 10^{2}\ \text{m}

    Stuck? Show hint

    Anchor to the visible spectrum: violet light has a wavelength of about 4×10−7 m4 \times 10^{-7}\ \text{m}.

    Show solution
    1. 1

      Anchor: visible light has wavelengths from about 4×10−7 m4 \times 10^{-7}\ \text{m} (violet) to 7×10−7 m7 \times 10^{-7}\ \text{m} (red).

      Ultraviolet sits just beyond the violet end of the spectrum — the name literally means "beyond violet", so it must be slightly shorter than violet's 4×10−74 \times 10^{-7} m.

    2. 2

      Ultraviolet wavelengths are therefore a little shorter than 4×10−7 m4 \times 10^{-7}\ \text{m}: an order of magnitude of 10−7 m10^{-7}\ \text{m} (ultraviolet runs from about 1×10−8 m1 \times 10^{-8}\ \text{m} to 4×10−7 m4 \times 10^{-7}\ \text{m}) — option B.

      The other options are far away: 10−1510^{-15} m is the size of a nucleus, 10−310^{-3} m is a microwave and 10210^{2} m a radio wave.

    Answer

    B — 1×10−7 m1 \times 10^{-7}\ \text{m} (ultraviolet runs from about 1×10−8 m1 \times 10^{-8}\ \text{m} up to 4×10−7 m4 \times 10^{-7}\ \text{m}).

02

SI base and derived units

Syllabus requirement · §1.2

“

recall the following SI base quantities and their units: mass (kg), length (m), time (s), current (A), temperature (K); express derived units as products or quotients of the SI base units and use the derived units for quantities listed in this syllabus as appropriate

”

Why a system of base units?

Rather than invent an independent unit for every quantity, SI builds everything from a handful of base quantities with agreed base units. Every other unit — newton, joule, volt, ohm — is then derived, meaning it can be written as a product or quotient of base units. Questions such as "determine the SI base units of …" check that you know where a unit comes from, not just its name.

Base quantity

SI base unit

mass

kilogram (kg)

length

metre (m)

time

second (s)

electric current

ampere (A)

temperature

kelvin (K)

Learn these five exactly. Note the kilogram — not the gram — is the base unit of mass. Two further base quantities exist (amount of substance, mole; luminous intensity, candela). Neither is examined directly at AS level — and when the mole does turn up inside an equation later on (ideal gases, at A Level), the method you learn here works on it unchanged.

Base quantity or not?

Only the five quantities in the table are base quantities in this course. Charge, force, energy, weight, speed and pressure are not — each is defined by an equation from other quantities (Q=ItQ = It, F=maF = ma, …), so each is derived. The favourite trap is charge: it feels basic, but the base electrical quantity is current, and charge is built from it.

The notation [X]

Square brackets around a quantity mean "the base unit of that quantity": [F][F] is read as "the unit of force". It keeps unit algebra visibly separate from number algebra. Units multiply, divide and cancel exactly like algebraic symbols — m/m=1\text{m}/\text{m} = 1, and m×m=m2\text{m} \times \text{m} = \text{m}^2.

Derived units are built, not memorised

Every other unit in physics is a derived unit: a product or quotient of base units, obtained by writing down the equation that defines the quantity and replacing each quantity by its unit. Build the seven you will meet most often, one line each, straight from the defining equation:

v=displacementt⟹[v]=ms=m s−1v = \frac{\text{displacement}}{t} \quad\Longrightarrow\quad [v] = \frac{\text{m}}{\text{s}} = \text{m s}^{-1} a=Δvt⟹[a]=m s−1s=m s−2a = \frac{\Delta v}{t} \quad\Longrightarrow\quad [a] = \frac{\text{m s}^{-1}}{\text{s}} = \text{m s}^{-2} F=ma⟹[F]=kg×m s−2=kg m s−2≡NF = ma \quad\Longrightarrow\quad [F] = \text{kg} \times \text{m s}^{-2} = \text{kg m s}^{-2} \equiv \text{N} p=FA⟹[p]=kg m s−2m2=kg m−1 s−2≡Pap = \frac{F}{A} \quad\Longrightarrow\quad [p] = \frac{\text{kg m s}^{-2}}{\text{m}^2} = \text{kg m}^{-1}\text{ s}^{-2} \equiv \text{Pa} W=Fd⟹[W]=kg m s−2×m=kg m2 s−2≡JW = Fd \quad\Longrightarrow\quad [W] = \text{kg m s}^{-2} \times \text{m} = \text{kg m}^2\text{ s}^{-2} \equiv \text{J} P=Wt⟹[P]=kg m2 s−2s=kg m2 s−3≡WP = \frac{W}{t} \quad\Longrightarrow\quad [P] = \frac{\text{kg m}^2\text{ s}^{-2}}{\text{s}} = \text{kg m}^2\text{ s}^{-3} \equiv \text{W} Q=It⟹[Q]=A×s=A s≡CQ = It \quad\Longrightarrow\quad [Q] = \text{A} \times \text{s} = \text{A s} \equiv \text{C}

Know the ≡\equiv relationships both ways round: sometimes you expand a named unit (the newton into kg m s−2\text{kg m s}^{-2}), sometimes you build an unfamiliar unit from scratch.

Expressing any derived unit in base units
  1. 1

    Write the defining equation for the quantity (or rearrange the given equation for it).

    Every derived unit traces back to a defining equation — if you do not know the equation, you cannot get the unit.

  2. 2

    Replace each quantity by its unit — a base unit if it has one (kg, m, s, A, K), or an already-known derived unit (N, J, …) that you then expand into base units.

  3. 3

    Simplify with index laws, cancelling anything that appears on top and bottom.

    Treat units as algebra: collect the powers of m, of s, and so on, one base unit at a time.

A clean demonstration

Find the base units of density ρ\rho.

Step 1 — defining equation: ρ=mV\rho = \dfrac{m}{V} (density is mass per unit volume).

Step 2 — replace each quantity by its unit: mass carries the base unit kg, volume carries the base unit m3\text{m}^3:

[ρ]=kgm3[\rho] = \frac{\text{kg}}{\text{m}^3}

Step 3 — simplify with index laws: dividing by m3\text{m}^3 gives

[ρ]=kg m−3[\rho] = \text{kg m}^{-3}

Short, but every step is there: equation → substitution → indices. That is the shape of every question of this type, no matter how buried the quantity is.

Base units of a constant buried inside an equation

9702/23 O/N 2025 Q2(b)(ii)

A small steel ball of radius rr and mass mm falls vertically at terminal speed vv through oil.

The viscous drag force DD that acts on the ball is given by

D=6πηrvD = 6\pi\eta rv

where η\eta is a property of the oil called its viscosity.

Determine the SI base units of η\eta.

Show full working
  1. 1

    Rearrange for η\eta: divide both sides of D=6πηrvD = 6\pi\eta rv by 6πrv6\pi rv:

    η=D6πrv\eta = \frac{D}{6\pi rv}

    Show the rearrangement explicitly — everything that follows reads the units off this line.

  2. 2

    The constant 6π6\pi is a pure number: it has no units and drops out of the unit analysis entirely.

    Only quantities with units contribute. Numbers are unit-free — forgetting this makes candidates try to assign units to 6π.

  3. 3

    Convert [D][D] to base units now: DD is a force, so [D]=N=kg m s−2[D] = \text{N} = \text{kg m s}^{-2} using the build of the newton from F=maF = ma earlier in this section.

    This conversion is where candidates who skip ahead stall later — leaving newtons unconverted means the final line cannot be finished. Convert to base units at the start, not the end.

  4. 4

    Write down the remaining pieces: rr is a radius, so [r]=m[r] = \text{m}; vv is a speed, so [v]=m s−1[v] = \text{m s}^{-1}.

  5. 5

    Substitute all three into the expression for η\eta:

    [η]=kg m s−2m×m s−1[\eta] = \frac{\text{kg m s}^{-2}}{\text{m} \times \text{m s}^{-1}}

    This substitution line earns its own mark (C1) on the mark scheme — write it out in full, never jump straight to the simplified result.

  6. 6

    Simplify each base unit with index laws. Length: m1\text{m}^{1} divided by (m1×m1)=m2(\text{m}^1 \times \text{m}^1) = \text{m}^2 gives m1−2=m−1\text{m}^{1-2} = \text{m}^{-1}. Time: s−2\text{s}^{-2} divided by s−1\text{s}^{-1} gives s−2−(−1)=s−1\text{s}^{-2-(-1)} = \text{s}^{-1}. So

    [η]=kg m−1 s−1[\eta] = \text{kg m}^{-1}\text{ s}^{-1}
Answer

η\eta has base units kg m−1 s−1\text{kg m}^{-1}\text{ s}^{-1}.

Convert every unit into base units before simplifying — a newton left sitting in the final line is the most common way to lose the answer mark here.

Your turn

The first checks the list of base quantities. The rest have the same shape every time: define (or rearrange), substitute units, simplify indices.

  1. 19702/22 F/M 2024 Q1(a)1 mark

    Table 1.1 lists some SI quantities. Complete the table by indicating with a tick (✓) which rows are SI base quantities.

    quantitybase quantity
    current
    energy
    force
    mass
    Show solution
    1. 1

      Check each row against the five base quantities: mass, length, time, current, temperature.

      Base quantities are a fixed list to recall, not something you work out.

    2. 2

      Current is on the list: tick.

    3. 3

      Energy is derived (from W=FdW = Fd, unit J=kg m2 s−2\text{J} = \text{kg m}^2\text{ s}^{-2}): no tick.

    4. 4

      Force is derived (from F=maF = ma, unit N=kg m s−2\text{N} = \text{kg m s}^{-2}): no tick.

    5. 5

      Mass is on the list: tick.

      The mark needs current and mass ticked and nothing else — one extra tick loses it.

    Answer

    Tick current and mass only.

  2. 29702/13 O/N 2025 Q22

    What are the SI base units of stress?

    Options

    A   kg m s−2\text{kg m s}^{-2}
    B   kg m−1 s−2\text{kg m}^{-1}\text{ s}^{-2}
    C   kg m−2 s−2\text{kg m}^{-2}\text{ s}^{-2}
    D   kg m−3 s−2\text{kg m}^{-3}\text{ s}^{-2}

    Stuck? Show hint

    Stress is defined as force per unit cross-sectional area.

    Show solution
    1. 1

      Stress is force per unit cross-sectional area. Write the defining equation: stress=forcearea⟹[stress]=[F][A]\text{stress} = \frac{\text{force}}{\text{area}} \quad\Longrightarrow\quad [\text{stress}] = \frac{[F]}{[A]}

    2. 2

      Put in the units: [F]=N=kg m s−2[F] = \text{N} = \text{kg m s}^{-2} (from F=maF = ma) and [A]=m2[A] = \text{m}^2, so [stress]=kg m s−2m2[\text{stress}] = \frac{\text{kg m s}^{-2}}{\text{m}^2}

      Expand the newton into base units before simplifying, or the answer cannot be written in base units.

    3. 3

      Simplify the length index only — mass and time carry straight down:
      [stress]=kg m1−2 s−2=kg m−1 s−2[\text{stress}] = \text{kg m}^{1-2}\text{ s}^{-2} = \text{kg m}^{-1}\text{ s}^{-2} — option B.

      Mass and time pass through untouched — only the length indices (one on top, two underneath) combine. Option A is the newton itself (the area was forgotten); C divides by m³ instead of m².

    Answer

    B — kg m−1 s−2\text{kg m}^{-1}\text{ s}^{-2} (the same as the pascal, built earlier in this section).

  3. 39702/12 O/N 2025 Q3

    Which physical quantity could have units of N s2 m−1\text{N s}^{2}\text{ m}^{-1}?

    Options

    A   acceleration
    B   force
    C   mass
    D   momentum

    Stuck? Show hint

    Expand the newton into base units first, then cancel the powers one base unit at a time.

    Show solution
    1. 1

      Expand the newton into base units: N=kg m s−2\text{N} = \text{kg m s}^{-2}, so

      N s2 m−1=kg m s−2×s2×m−1\text{N s}^2\text{ m}^{-1} = \text{kg m s}^{-2} \times \text{s}^2 \times \text{m}^{-1}

      Convert the newton first — every cancellation that follows reads straight off that expansion.

    2. 2

      Collect each base unit. Length: m1×m−1=m0\text{m}^{1} \times \text{m}^{-1} = \text{m}^{0} — cancels completely. Time: s−2×s2=s0\text{s}^{-2} \times \text{s}^{2} = \text{s}^{0} — cancels completely.

    3. 3

      All that survives is kg\text{kg} — the base unit of mass, option C.

    4. 4

      Check the others against their own base units: acceleration is m s−2\text{m s}^{-2}, force is kg m s−2\text{kg m s}^{-2} and momentum is kg m s−1\text{kg m s}^{-1} (=N s= \text{N s}) — none of them is a bare kg\text{kg}.

      Momentum is the tempting distractor because it too can be written with a newton in it (N s), but it keeps one metre and one second that this unit has cancelled away.

    Answer

    C — mass (N s2 m−1=kg m s−2×s2×m−1=kg\text{N s}^2\text{ m}^{-1} = \text{kg m s}^{-2} \times \text{s}^2 \times \text{m}^{-1} = \text{kg}).

  4. 4

    Potential difference is defined by V=WQV = \dfrac{W}{Q}, where WW is energy and QQ is charge. Express the volt in SI base units.

    Stuck? Show hint

    You need two expansions from this section: the joule and the coulomb.

    Show solution
    1. 1

      From the definition: [V]=[W][Q][V] = \frac{[W]}{[Q]} so the volt must be built from the units of energy and charge.

      Both named units on the right must be in base-unit form before dividing — comparing joules and coulombs directly proves nothing.

    2. 2

      Expand the energy unit from its build earlier in this section: [W]=J=N m=(kg m s−2)×m=kg m2 s−2[W] = \text{J} = \text{N m} = (\text{kg m s}^{-2}) \times \text{m} = \text{kg m}^2\text{ s}^{-2}

    3. 3

      Expand the charge unit: [Q]=C=A s[Q] = \text{C} = \text{A s} (from Q=ItQ = It).

    4. 4

      Substitute both: [V]=kg m2 s−2A s[V] = \frac{\text{kg m}^2\text{ s}^{-2}}{\text{A s}}

    5. 5

      Simplify one base unit at a time. Time: s−2\text{s}^{-2} divided by s1\text{s}^{1} gives s−2−1=s−3\text{s}^{-2-1} = \text{s}^{-3}. The ampere on the bottom becomes A−1\text{A}^{-1}. So [V]=kg m2 s−3 A−1[V] = \text{kg m}^2\text{ s}^{-3}\text{ A}^{-1}

      Nothing cancels the ampere, so it stays in the answer with a negative power.

    Answer

    kg m2 s−3 A−1\text{kg m}^2\text{ s}^{-3}\text{ A}^{-1}

In the exam
108 question parts · 71 Paper 1 + 37 Paper 2 · 2021–2025

From 2021 to 2025, 108 question parts on Papers 1 and 2 tested base units, derived units or homogeneity (71 on Paper 1, 37 on Paper 2) — the largest share of this topic. Base units also turn up inside later topics, so this skill is worth making automatic.

03

Prefixes: pico to tera

Syllabus requirement · §1.2

“

recall and use the following prefixes and their symbols to indicate decimal submultiples or multiples of both base and derived units: pico (p), nano (n), micro (μ), milli (m), centi (c), deci (d), kilo (k), mega (M), giga (G), tera (T)

”

Why prefixes exist

Physics numbers span an enormous range — light has wavelengths of a few hundred nanometres, while a power station delivers gigawatts. Prefixes attach a power of ten to a unit so the number in front stays a sensible size. Two skills are examined: rewriting a value with a friendlier prefix, and converting a compound unit (one with a prefix in it, like kN mm−2\text{kN mm}^{-2}) into plain base units. Both reduce to the same move: replace the prefix by its power of ten and let the indices do the work.

Prefix

Symbol

Multiple

pico

p

10−1210^{-12}

nano

n

10−910^{-9}

micro

μ

10−610^{-6}

milli

m

10−310^{-3}

centi

c

10−210^{-2}

deci

d

10−110^{-1}

kilo

k

10310^{3}

mega

M

10610^{6}

giga

G

10910^{9}

tera

T

101210^{12}

Case matters: m is milli (10⁻³) but M is mega (10⁶). And μ (micro) is nothing like m (milli) — 1 μm is a thousand times smaller than 1 mm.

The squared-prefix trap

A prefix attaches to the unit, and then any index squares (or cubes) the whole thing:

1 cm2=(1 cm)2=(10−2 m)2=10−4 m21\ \text{cm}^2 = (1\ \text{cm})^2 = (10^{-2}\ \text{m})^2 = 10^{-4}\ \text{m}^2

not 10−2 m210^{-2}\ \text{m}^2. The same applies to mm2\text{mm}^2, cm3\text{cm}^3 and every other prefixed unit carrying an index — the index acts on the power of ten too.

Converting a compound unit
  1. 1

    Replace each prefix with its power of ten, keeping the unit it is attached to.

    One prefix at a time — a value like kN mm⁻² has two independent replacements to make.

  2. 2

    Collect the powers of ten, remembering that any index on the unit applies to its power of ten as well.

    This is the squared-prefix trap from the callout: (10−3)−2=106(10^{-3})^{-2} = 10^{6}, not 10310^{3}.

  3. 3

    Recombine into standard form (a single digit times a power of ten).

Two quick demonstrations

Removing a prefix. Convert the wavelength 450 nm450\ \text{nm} (nanometres) into metres. Replace n by 10−910^{-9}:

450 nm=450×10−9 m450\ \text{nm} = 450 \times 10^{-9}\ \text{m}

Then write it in standard form (one digit before the point):

450×10−9 m=4.5×10−7 m450 \times 10^{-9}\ \text{m} = 4.5 \times 10^{-7}\ \text{m}

A squared prefix. Convert 25 cm225\ \text{cm}^2 into m2\text{m}^2. Replace c by 10−210^{-2}, then square:

25 cm2=25×(10−2 m)2=25×10−4 m2=2.5×10−3 m225\ \text{cm}^2 = 25 \times (10^{-2}\ \text{m})^2 = 25 \times 10^{-4}\ \text{m}^2 = 2.5 \times 10^{-3}\ \text{m}^2

Notice the index 22 acting on the 10−210^{-2}: that is the entire trap in one line.

A compound unit with two prefixes

9702/12 M/J 2025 Q2

What is 0.25 kN mm−20.25\ \text{kN mm}^{-2} expressed in N m−2\text{N m}^{-2}?

Options

A   0.00025 N m−20.00025\ \text{N m}^{-2}
B   0.25 N m−20.25\ \text{N m}^{-2}
C   250 000 N m−2250\,000\ \text{N m}^{-2}
D   250 000 000 N m−2250\,000\,000\ \text{N m}^{-2}

Show full working
  1. 1

    Replace the first prefix: k=103k = 10^{3}, so

    0.25 kN=0.25×103 N0.25\ \text{kN} = 0.25 \times 10^{3}\ \text{N}

    One prefix at a time, exactly as in the method.

  2. 2

    Replace the second: mm (milli) =10−3= 10^{-3}, so 1 mm=10−3 m1\ \text{mm} = 10^{-3}\ \text{m}, and therefore

    1 mm−2=(10−3 m)−21\ \text{mm}^{-2} = (10^{-3}\ \text{m})^{-2}

    The prefix belongs to the metre, and the index −2-2 squares the whole 10−310^{-3} — this is the step everything hinges on.

  3. 3

    Simplify that power: (10−3)−2=10(−3)×(−2)=106(10^{-3})^{-2} = 10^{(-3) \times (-2)} = 10^{6}, so 1 mm−2=106 m−21\ \text{mm}^{-2} = 10^{6}\ \text{m}^{-2}.

    Forgetting to square the power of ten is THE error on this question — taking 1 mm2=10−3 m21\ \text{mm}^2 = 10^{-3}\ \text{m}^2 instead of 10−6 m210^{-6}\ \text{m}^2 produces the trap answer 2.5×1052.5 \times 10^{5}.

  4. 4

    Combine both replacements:

    0.25 kN mm−2=0.25×103×106 N m−20.25\ \text{kN mm}^{-2} = 0.25 \times 10^{3} \times 10^{6}\ \text{N m}^{-2}
  5. 5

    Collect the powers of ten and recombine into standard form:
    0.25×109 N m−2=2.5×108 N m−2=250 000 000 N m−20.25 \times 10^{9}\ \text{N m}^{-2} = 2.5 \times 10^{8}\ \text{N m}^{-2} = 250\,000\,000\ \text{N m}^{-2} — option D.

Answer

D — 250 000 000 N m−2250\,000\,000\ \text{N m}^{-2} (=2.5×108 N m−2= 2.5 \times 10^{8}\ \text{N m}^{-2})

Whenever a prefixed unit carries an index, the power of ten gets the same index — (10−3)−2=106(10^{-3})^{-2} = 10^{6}, never 10310^{3}.

Your turn

  1. 19702/13 M/J 2024 Q1

    What is equal to 0.000005 J0.000005\ \text{J}?

    Options

    A   5 mJ5\ \text{mJ}
    B   5 MJ5\ \text{MJ}
    C   5 μJ5\ \mu\text{J}
    D   5 nJ5\ \text{nJ}

    Show solution
    1. 1

      Count the places the decimal point must move to put a single digit in front: 0.000005=5×10−6 J0.000005 = 5 \times 10^{-6}\ \text{J} (six places).

    2. 2

      Match the power of ten to a prefix: 10−610^{-6} is micro, symbol μ. 5×10−6 J=5 μJ5 \times 10^{-6}\ \text{J} = 5\ \mu\text{J} — option C.

      mJ is 10−310^{-3} (too big), nJ is 10−910^{-9} (too small), and MJ (capital M) is 10610^{6} — the case of the letter matters.

    Answer

    C — 5 μJ5\ \mu\text{J}

  2. 2

    Express the resistance 4.7 GΩ4.7\ \text{G}\Omega (a) in MΩ\text{M}\Omega, (b) in Ω\Omega.

    Stuck? Show hint

    109/106=10310^{9} / 10^{6} = 10^{3} — how many mega-units fit into one giga-unit?

    Show solution
    1. 1

      (a) Replace G by 10910^{9}: 4.7 GΩ=4.7×109 Ω4.7\ \text{G}\Omega = 4.7 \times 10^{9}\ \Omega

      Going through plain ohms first means you only ever need one prefix at a time.

    2. 2

      One megaohm is 106 Ω10^{6}\ \Omega, so divide by 10610^{6} to count megaohms: 4.7×109106=4.7×103 MΩ=4700 MΩ\frac{4.7 \times 10^{9}}{10^{6}} = 4.7 \times 10^{3}\ \text{M}\Omega = 4700\ \text{M}\Omega

    3. 3

      (b) Straight from the replacement: 4.7 GΩ=4.7×109 Ω4.7\ \text{G}\Omega = 4.7 \times 10^{9}\ \Omega

    Answer

    (a) 4700 MΩ4700\ \text{M}\Omega (b) 4.7×109 Ω4.7 \times 10^{9}\ \Omega

  3. 3

    A wire has a diameter of 0.80 mm0.80\ \text{mm}. Taking its cross-section to be circular, express its cross-sectional area in m2\text{m}^2.

    Stuck? Show hint

    A=πd2/4A = \pi d^2 / 4 — and the squared-prefix trap applies to (0.80×10−3)2(0.80 \times 10^{-3})^2.

    Show solution
    1. 1

      Convert the diameter to metres first: d=0.80 mm=0.80×10−3 m=8.0×10−4 md = 0.80\ \text{mm} = 0.80 \times 10^{-3}\ \text{m} = 8.0 \times 10^{-4}\ \text{m}

    2. 2

      Square it, applying the index to the power of ten: d2=(8.0×10−4)2=64×10−8=6.4×10−7 m2d^2 = (8.0 \times 10^{-4})^2 = 64 \times 10^{-8} = 6.4 \times 10^{-7}\ \text{m}^2

    3. 3

      Substitute into the circle formula A=πd24A = \dfrac{\pi d^2}{4}: A=π×6.4×10−74A = \frac{\pi \times 6.4 \times 10^{-7}}{4}

    4. 4

      Evaluate: A=3.1416×6.4×10−74=5.0×10−7 m2A = \frac{3.1416 \times 6.4 \times 10^{-7}}{4} = 5.0 \times 10^{-7}\ \text{m}^2 (to 2 s.f., matching the data).

    Answer

    A≈5.0×10−7 m2A \approx 5.0 \times 10^{-7}\ \text{m}^2

04

Checking equations with base units

Syllabus requirement · §1.2

“

use SI base units to check the homogeneity of physical equations

”

Equations must balance in units too

Units multiply, divide and cancel exactly like algebraic symbols — so an equation has two things to balance: the numbers and the units. An equation whose two sides carry the same base units is called homogeneous. A physically possible equation must be homogeneous: you can never add a velocity to an energy any more than you can add 3 apples to 5 minutes.

This gives you a genuinely useful weapon:

  • if an equation is not homogeneous, it is definitely wrong — no exceptions;
  • on a multiple-choice paper that alone eliminates options;
  • rearranged, it finds the base units of a constant hiding inside an equation (as in the viscosity example in “SI base and derived units”);
  • it can find an unknown power in an equation (shown below).
Homogeneous ≠ correct

Homogeneity is a one-way test. If both sides match in base units the equation is possible — but it might still be wrong: a factor of 22 in the wrong place, or a ++ where there should be a −-, survives a units check perfectly. What homogeneity guarantees is only the other direction: not homogeneous = certainly wrong.

Checking an equation for homogeneity
  1. 1

    Replace every quantity on both sides by its base units. Pure numbers (22, π\pi, 12\tfrac{1}{2}) have no units; a named constant may carry units of its own.

    Every quantity, on both sides — including anything inside a root or a bracket. Missing one quantity is the usual way this check goes wrong.

  2. 2

    Simplify each side with index laws until each side is a single product like kg m s−1\text{kg m s}^{-1}.

    If an equation adds terms, each term must be simplified and compared separately.

  3. 3

    Compare the sides. Same base units → homogeneous (possible). Different → the equation is definitely wrong.

A clean demonstration

Check that v2=u2+2asv^2 = u^2 + 2as is homogeneous. (This is an equation of motion from the AS Kinematics note: uu and vv are speeds, aa is an acceleration and ss is a distance. You only need their units here.)

Left-hand side: [v2]=(m s−1)2=m2 s−2[v^2] = (\text{m s}^{-1})^2 = \text{m}^2\text{ s}^{-2}.

Right-hand side, term by term (an equation with a ++ needs every term checked against the other side):

  • [u2]=(m s−1)2=m2 s−2[u^2] = (\text{m s}^{-1})^2 = \text{m}^2\text{ s}^{-2} ✓
  • [2as][2as]: the 22 is a pure number with no units, so [2as]=[a][s]=(m s−2)×m=m2 s−2[2as] = [a][s] = (\text{m s}^{-2}) \times \text{m} = \text{m}^2\text{ s}^{-2} ✓

Every term matches m2 s−2\text{m}^2\text{ s}^{-2}, so the equation is homogeneous — it could be correct. (Whether it actually is correct is a matter of physics, not units.)

Which mass-on-a-spring formula could be right?

9702/12 F/M 2024 Q3

An object of mass mm is suspended by a spring from a fixed point. The spring has spring constant kk, and the object is set into vertical oscillations of period TT. Which equation for TT is homogeneous with respect to base units?

Options

A   T=2πkmT = 2\pi\dfrac{k}{m}
B   T=2πmkT = 2\pi\dfrac{m}{k}
C   T=2πkmT = 2\pi\sqrt{\dfrac{k}{m}}
D   T=2πmkT = 2\pi\sqrt{\dfrac{m}{k}}

Fig. 1 from the question paper.

Fig. 1 from the question paper.

Show full working
  1. 1

    The answer must come out in seconds: [T]=s[T] = \text{s} so whichever combination of kk and mm simplifies to s\text{s} is the homogeneous one.

    Fixing the target unit first tells you what you are hunting for.

  2. 2

    Find [k][k] from its defining equation. The spring constant is defined by Hooke's law F=kxF = kx, so k=Fx⟹[k]=kg m s−2m=kg s−2k = \frac{F}{x} \quad\Longrightarrow\quad [k] = \frac{\text{kg m s}^{-2}}{\text{m}} = \text{kg s}^{-2}

    kk is not a base quantity — its unit must be built from the equation that defines it, exactly as in “SI base and derived units”.

  3. 3

    Test A: [km]=kg s−2kg=s−2\left[\dfrac{k}{m}\right] = \dfrac{\text{kg s}^{-2}}{\text{kg}} = \text{s}^{-2}. That is not s\text{s}, so A fails.

  4. 4

    Test B: [mk]=kgkg s−2=s2\left[\dfrac{m}{k}\right] = \dfrac{\text{kg}}{\text{kg s}^{-2}} = \text{s}^{2}. Not s\text{s}, so B fails.

    Note how close B looks to D — same ingredients, but no square root. Units do not care about closeness: s² ≠ s.

  5. 5

    Test C: simplify the fraction inside the root first, [km]=s−2\left[\dfrac{k}{m}\right] = \text{s}^{-2}, then take the root: (s−2)1/2=s−1(\text{s}^{-2})^{1/2} = \text{s}^{-1}. Not s\text{s}, so C fails.

  6. 6

    Test D: the fraction is again s2\text{s}^{2} (step 4), and taking the square root gives (s2)1/2=s(\text{s}^{2})^{1/2} = \text{s} ✓. This matches [T][T], so D is the homogeneous equation.

Answer

D — T=2πm/kT = 2\pi\sqrt{m/k} (the only option whose base units simplify to seconds).

When testing roots, simplify the fraction's units first and take the root second — trying to do both at once is where slips happen.

Finding an unknown power

Sometimes the equation contains an unknown power nn, and you are told the equation is homogeneous. Then the powers of each base unit must be equal on both sides, and that gives an equation for nn.

Demonstration. The kinetic energy of a moving object is E=12mvnE = \tfrac{1}{2}mv^n. Find nn.

Left-hand side: energy is measured in joules, [E]=kg m2 s−2[E] = \text{kg m}^2\text{ s}^{-2}.

Right-hand side: the 12\tfrac{1}{2} has no units, so

[mvn]=kg×(m s−1)n=kg mn s−n[mv^n] = \text{kg} \times (\text{m s}^{-1})^n = \text{kg m}^{n}\text{ s}^{-n}

(the power nn acts on every unit inside the bracket).

Match the metres: m2\text{m}^2 on the left and mn\text{m}^n on the right, so n=2n = 2.

Check with the seconds: s−2\text{s}^{-2} on the left and s−n=s−2\text{s}^{-n} = \text{s}^{-2} on the right ✓. The kilograms already match. So E=12mv2E = \tfrac{1}{2}mv^2.

Your turn

Build each candidate side term by term; pure numbers never contribute units.

  1. 19702/12 M/J 2025 Q4

    The time period TT of a pendulum is given by

    T=2π(Lg)nT = 2\pi\left(\frac{L}{g}\right)^n

    where LL is the length of the pendulum and gg is the acceleration of free fall. The equation is homogeneous. What is the value of nn?

    Options

    A   −2-2
    B   −12-\tfrac{1}{2}
    C   12\tfrac{1}{2}
    D   22

    Stuck? Show hint

    Simplify the units of L/gL/g first, then ask what power turns them into seconds.

    Show solution
    1. 1

      The left-hand side is a time: [T]=s[T] = \text{s}. The 2π2\pi is a pure number with no units.

    2. 2

      Units inside the bracket: [L]=m[L] = \text{m} and [g]=m s−2[g] = \text{m s}^{-2}, so [Lg]=mm s−2=s2\left[\frac{L}{g}\right] = \frac{\text{m}}{\text{m s}^{-2}} = \text{s}^{2}

      The metres cancel, and dividing by s−2\text{s}^{-2} is the same as multiplying by s2\text{s}^{2}.

    3. 3

      Raise to the power nn: [(Lg)n]=(s2)n=s2n\left[\left(\frac{L}{g}\right)^n\right] = (\text{s}^{2})^n = \text{s}^{2n}

    4. 4

      Match the powers of seconds on both sides: s1=s2n⟹2n=1⟹n=12\text{s}^{1} = \text{s}^{2n} \quad\Longrightarrow\quad 2n = 1 \quad\Longrightarrow\quad n = \tfrac{1}{2} — option C.

      n=−12n = -\tfrac{1}{2} (option B) would give s−1\text{s}^{-1}, a frequency, not a time. A power of 12\tfrac{1}{2} is a square root, so this is T=2πL/gT = 2\pi\sqrt{L/g}.

    Answer

    C — n=12n = \tfrac{1}{2}, so T=2πL/gT = 2\pi\sqrt{L/g}.

  2. 29702/11 O/N 2019 Q2

    The speed of a wave in deep water depends on its wavelength LL and the acceleration of free fall gg. What is a possible equation for the speed vv of the wave?

    Options

    A   v=gL2πv = \sqrt{\dfrac{gL}{2\pi}}
    B   v=gL4π2v = \dfrac{gL}{4\pi^2}
    C   v=2πgLv = 2\pi\sqrt{\dfrac{g}{L}}
    D   v=2πgLv = \dfrac{2\pi g}{L}

    Show solution
    1. 1

      Write down what the answer must reduce to: [v]=m s−1[v] = \text{m s}^{-1}. The ingredients are [L]=m[L] = \text{m} and [g]=m s−2[g] = \text{m s}^{-2}; 2π2\pi and 4π24\pi^2 are pure numbers with no units.

    2. 2

      Test A: gL=(m s−2)×m=m2 s−2gL = (\text{m s}^{-2}) \times \text{m} = \text{m}^2\text{ s}^{-2}; dividing by 2π2\pi changes nothing; taking the square root gives m s−1\text{m s}^{-1} ✓ — A works.

    3. 3

      Test B: the same product gL=m2 s−2gL = \text{m}^2\text{ s}^{-2}, but with no square root this time ✗.

      B is A without the root — a reminder that the root is doing real work on the indices, halving both of them.

    4. 4

      Test C: gL=m s−2m=s−2\dfrac{g}{L} = \dfrac{\text{m s}^{-2}}{\text{m}} = \text{s}^{-2}; square root gives s−1\text{s}^{-1} ✗.

      The result has no metre in it at all — a speed needs both m and s, so C fails despite looking plausible.

    5. 5

      Test D: gL=s−2\dfrac{g}{L} = \text{s}^{-2} again, with no root to fix it ✗.

    6. 6

      Only A reduces to m s−1\text{m s}^{-1}.

    Answer

    A — v=gL/2πv = \sqrt{gL/2\pi}

  3. 39702/12 M/J 2019 Q3

    The Planck constant hh has SI units J s.

    Which equation could be used to calculate the Planck constant?

    Options

    A   h=DEvh = \dfrac{DE}{v} where DD is distance, EE is energy and vv is velocity
    B   h=vDh = \dfrac{v}{D} where vv is velocity and DD is distance
    C   h=14πEh = \dfrac{1}{4\pi E} where EE is electric field strength
    D   h=Fr2mh = \dfrac{Fr^2}{m} where FF is force, rr is radius and mm is mass

    Stuck? Show hint

    Read each option's own definitions before testing it — the EE in A and the EE in C are different quantities.

    Show solution
    1. 1

      Put the target into base units first: J=kg m2 s−2\text{J} = \text{kg m}^2\text{ s}^{-2}, so [h]=J s=kg m2 s−2×s=kg m2 s−1[h] = \text{J s} = \text{kg m}^2\text{ s}^{-2} \times \text{s} = \text{kg m}^2\text{ s}^{-1}

      Every option will be reduced to base units, so the target must be in base units too.

    2. 2

      Convert the named derived units option by option. In A, EE is an energy: [E]=J=kg m2 s−2[E] = \text{J} = \text{kg m}^2\text{ s}^{-2}. In D, [F]=N=kg m s−2[F] = \text{N} = \text{kg m s}^{-2}. Also [D]=[r]=m[D] = [r] = \text{m}, [v]=m s−1[v] = \text{m s}^{-1}, and [m]=kg[m] = \text{kg}.

      Each option supplies its own key — testing all four with one blanket meaning for E would test the wrong physics in C.

    3. 3

      Test A: build up piece by piece.

      [D][E]=m×kg m2 s−2=kg m3 s−2[D][E] = \text{m} \times \text{kg m}^2\text{ s}^{-2} = \text{kg m}^3\text{ s}^{-2}

      then divide by [v][v]:
      kg m3 s−2m s−1=kg m3−1 s−2−(−1)=kg m2 s−1✓\frac{\text{kg m}^3\text{ s}^{-2}}{\text{m s}^{-1}} = \text{kg m}^{3-1}\text{ s}^{-2-(-1)} = \text{kg m}^2\text{ s}^{-1} ✓ — matches [h][h].

      Numerator simplified first, then divided — the same two-pass habit as simplifying any algebraic fraction.

    4. 4

      Test B: [v][D]=m s−1m=s−1\dfrac{[v]}{[D]} = \dfrac{\text{m s}^{-1}}{\text{m}} = \text{s}^{-1} ✗.

    5. 5

      Test C: here EE is electric field strength, which is force per unit charge, E=F/QE = F/Q (you meet it properly later in the course). Build its unit, using [Q]=A s[Q] = \text{A s}:

      [E]=kg m s−2A s=kg m s−3 A−1[E] = \frac{\text{kg m s}^{-2}}{\text{A s}} = \text{kg m s}^{-3}\text{ A}^{-1}

      Inverting, 14π[E]=kg−1 m−1 s3 A\dfrac{1}{4\pi[E]} = \text{kg}^{-1}\text{ m}^{-1}\text{ s}^{3}\text{ A} ✗ (the 4π4\pi contributes nothing).

      Inverting a unit flips the sign of every index — and a negative kilogram index alone already kills it, because h carries kg to the power +1.

    6. 6

      Test D: [F][r]2=(kg m s−2)×m2=kg m3 s−2[F][r]^2 = (\text{kg m s}^{-2}) \times \text{m}^2 = \text{kg m}^3\text{ s}^{-2}; dividing by [m][m]:
      kg m3 s−2kg=m3 s−2\frac{\text{kg m}^3\text{ s}^{-2}}{\text{kg}} = \text{m}^3\text{ s}^{-2} ✗

      The kilograms cancel completely, but hh needs kg1\text{kg}^{1} — so D fails even before you look at the metres and seconds.

    Answer

    A — h=DE/vh = DE/v

  4. 4

    The ideal-gas equation pV=nRTpV = nRT is homogeneous. Given [p]=kg m−1 s−2[p] = \text{kg m}^{-1}\text{ s}^{-2}, [V]=m3[V] = \text{m}^3, nn is an amount in mol and TT is a temperature in K, determine the base units of RR.

    Show solution
    1. 1

      Rearrange for RR: R=pVnT⟹[R]=[p][V][n][T]R = \frac{pV}{nT} \quad\Longrightarrow\quad [R] = \frac{[p][V]}{[n][T]}

    2. 2

      Combine pressure and volume first: [p][V]=(kg m−1 s−2)×m3=kg m−1+3 s−2=kg m2 s−2[p][V] = (\text{kg m}^{-1}\text{ s}^{-2}) \times \text{m}^3 = \text{kg m}^{-1+3}\text{ s}^{-2} = \text{kg m}^2\text{ s}^{-2}

    3. 3

      Divide by mol and kelvin — neither cancels with anything above:

      [R]=kg m2 s−2mol×K=kg m2 s−2 K−1 mol−1[R] = \frac{\text{kg m}^2\text{ s}^{-2}}{\text{mol} \times \text{K}} = \text{kg m}^2\text{ s}^{-2}\text{ K}^{-1}\text{ mol}^{-1}

      Mol and kelvin are base units in their own right — nothing upstairs cancels them, so they ride along into the answer.

    Answer

    kg m2 s−2 K−1 mol−1\text{kg m}^2\text{ s}^{-2}\text{ K}^{-1}\text{ mol}^{-1}

05

Systematic and random errors; precision and accuracy

Syllabus requirement · §1.3

“

understand and explain the effects of systematic errors (including zero errors) and random errors in measurements; understand the distinction between precision and accuracy

”

No measurement is perfect

Every reading you take is slightly wrong. What matters — in the exam and in a real experiment — is how it is wrong. Errors come in two kinds that behave very differently, and you must use the four words of this section (random, systematic, precise, accurate) exactly.

Random errors: scatter both ways

A random error makes repeated readings scatter unpredictably on both sides of the true value — sometimes high, sometimes low. Typical causes:

  • judging a scale mark with your eye at a slightly different angle each time (parallax that varies),
  • human reaction time when timing with a stopwatch,
  • fluctuations in the quantity itself (a draught nudging a thermometer).

Random errors reduce precision: the repeats disagree with each other. Their effect shrinks when you average several readings — the highs and lows partially cancel, so the mean lands closer to the truth than any single reading.

Systematic errors: everything shifted the same way

A systematic error pushes every reading the same direction by roughly the same amount. Typical causes:

  • a zero error — a balance reading 0.2 g0.2\ \text{g} before anything is placed on it, or closed calipers not reading exactly zero,
  • a rule worn short at one end,
  • a thermometer consistently reading 1 ∘1\ ^\circC high.

Because every reading shifts together, repeating and averaging does nothing to a systematic error — the mean of many shifted readings is still shifted. It must be attacked at the source: check the instrument against a known value (calibration), subtract the zero reading, or use a different technique.

Correcting a zero error. Closed calipers read 0.03 mm0.03\ \text{mm} instead of zero. A wire then reads 5.27 mm5.27\ \text{mm}. Every reading is 0.03 mm0.03\ \text{mm} too big, so subtract the zero reading:

d=5.27−0.03=5.24 mmd = 5.27 - 0.03 = 5.24\ \text{mm}

If the closed reading were −0.03 mm-0.03\ \text{mm} (below zero), you would subtract −0.03-0.03, which means adding 0.03 mm0.03\ \text{mm}.

12345678reading numbertrue value12345678reading numbertrue valuemeanRandom errorscatter either side of the true valuemean sits on the true value — averaging helpsmeanSystematic errorevery reading shifted the SAME wayrepeating and averaging will NOT fix it

Repeated readings plotted against reading number: random errors scatter either side of the true line (averaging helps); a systematic error rides a constant offset above it (averaging changes nothing).

Repeating fixes random, never systematic

Remember this sentence: taking repeat readings and averaging reduces the effect of random errors only. A systematic error survives averaging perfectly intact — it can only be found by checking against a known value or eliminating the zero.

Precision and accuracy are different words for different things

  • Precision describes how close the repeats are to each other — small scatter means precise.
  • Accuracy describes how close the mean is to the true value.

The two are independent, and the interesting case is a data set that is precise but inaccurate: a tight cluster sitting in the wrong place. That pattern is the signature of a systematic error — the readings agree beautifully with each other because they are all wrong by the same amount.

precise and accuratetight cluster, on the true valueprecise, not accuratetight, but off target — systematicaccurate, not precisescattered about true value — randomneither precise nor accuratescattered, and shifted off targettrue value

Four targets, four diagnoses: precise and accurate (tight cluster centred), precise but inaccurate (tight cluster off-centre — the systematic-error signature), imprecise but accurate on average (wide scatter centred), and neither.

A clean demonstration

A student measures the length of a wire five times with the same rule:

30.2,30.4,30.2,30.3,30.4 cm30.2,\quad 30.4,\quad 30.2,\quad 30.3,\quad 30.4\ \text{cm}

Precision. The spread is 30.4−30.2=0.2 cm30.4 - 30.2 = 0.2\ \text{cm}. The repeats agree closely with each other, so the set is precise.

Accuracy. The mean is

xˉ=30.2+30.4+30.2+30.3+30.45=151.55=30.3 cm\bar{x} = \frac{30.2 + 30.4 + 30.2 + 30.3 + 30.4}{5} = \frac{151.5}{5} = 30.3\ \text{cm}

Now suppose the first 0.3 cm0.3\ \text{cm} of the rule has worn away, and the student lines the wire up with the worn end. The end of the rule is now really at the 0.3 cm0.3\ \text{cm} mark, so every reading comes out 0.3 cm0.3\ \text{cm} too high. The true length is then 30.3−0.3=30.0 cm30.3 - 0.3 = 30.0\ \text{cm}, and the mean of 30.3 cm30.3\ \text{cm} misses it by 0.3 cm0.3\ \text{cm}: the set is inaccurate despite being precise. Tight cluster, wrong place — the systematic-error signature, exactly as in the targets diagram.

Accurate AND precise? Check them separately

9702/14 O/N 2025 Q2

A steel rule can be read to the nearest millimetre. It is used to measure the length of a bar whose true length is 895 mm895\ \text{mm}. Repeated measurements give the following readings.

length / mm
892, 891, 892, 891, 891, 892

Are the readings accurate and precise to within 1 mm1\ \text{mm}?

Options

results are accurate to within 1 mm1\ \text{mm}results are precise to within 1 mm1\ \text{mm}
Anono
Bnoyes
Cyesno
Dyesyes
Show full working
  1. 1

    Precision first — compare the repeats with each other. Spread == largest −- smallest =892−891=1 mm= 892 - 891 = 1\ \text{mm}, which is within 1 mm1\ \text{mm}: the readings are precise.

    Precision needs only the spread of the repeats — no mean, no true value yet.

  2. 2

    Now the mean, one piece at a time: 892+891+892+891+891+892=5349892 + 891 + 892 + 891 + 891 + 892 = 5349 xˉ=53496=891.5 mm\bar{x} = \frac{5349}{6} = 891.5\ \text{mm}

  3. 3

    Accuracy — compare the mean with the true value: ∣895−891.5∣=3.5 mm|895 - 891.5| = 3.5\ \text{mm} which is larger than 1 mm1\ \text{mm}: the readings are not accurate.

  4. 4

    Conclusion: accurate no, precise yes — option B. The readings form a tight cluster about 3.5 mm3.5\ \text{mm} below the truth, the classic signature of a systematic error such as a zero error shifting every reading down.

    The two judgements are independent: choosing D ("both") comes from checking precision and assuming accuracy follows. It never does automatically.

Answer

B — not accurate (the mean of 891.5 mm891.5\ \text{mm} is 3.5 mm3.5\ \text{mm} from the true 895 mm895\ \text{mm}) but precise (spread of only 1 mm1\ \text{mm} between repeats).

Always run the two checks separately: spread of repeats for precision, then distance of the mean from the true value for accuracy.

Your turn

For every statement, ask: does this behave differently for random and for systematic?

  1. 19702/13 M/J 2025 Q3

    Which statement about errors in measurements is correct?

    Options

    A   An accurate set of measurements always has a small random error.
    B   A precise set of measurements always has a small systematic error.
    C   A random error can be reduced by taking an average of several measurements.
    D   A systematic error creates a random set of measurements spread out about the true value.

    Show solution
    1. 1

      A fails: accuracy is about the mean sitting on the true value. A set can scatter widely (large random error) and still average out accurately, so accuracy does not guarantee a small random error.

    2. 2

      B fails: precision is about the spread only. A tightly clustered set sitting far from the true value is precise with a large systematic error — the two ideas are independent.

      This is the classic trap: precision says nothing about where the cluster sits, only how tight it is.

    3. 3

      C works: random errors scatter either side of the true value, so averaging lets the highs and lows cancel — the standard remedy.

    4. 4

      D fails: a systematic error moves the whole cluster sideways by the same amount each time; it does not create scatter, and the readings are no longer spread about the true value.

    Answer

    C — averaging several measurements reduces random errors only.

  2. 29702/12 O/N 2025 Q2

    What describes a set of data with a high precision?

    Options

    A   data measured using equipment with small scale divisions
    B   data that is close to the accepted value
    C   data with each value having a low uncertainty
    D   data with repeats that are close to each other

    Show solution
    1. 1

      High precision means the measured values are close to each other — the spread (scatter) between repeat readings is small. That is option D.

      Close to each other, not close to the true value: closeness to the truth is accuracy.

    2. 2

      B fails: close to the accepted value describes accuracy. A and C fail: small scale divisions and low uncertainty describe the instrument's resolution, not how well repeated readings agree.

    Answer

    D — data with repeats that are close to each other.

  3. 39702/21 O/N 2024 Q1(c)

    Fig. 1.1 shows a cuboidal glass block.

    A student measures the mass mm of the block and the side lengths xx, yy and zz. The measurements are shown in Table 1.1.

    quantitymeasurement
    mm(0.243±0.001) kg(0.243 \pm 0.001)\ \text{kg}
    xx(5.41±0.01) cm(5.41 \pm 0.01)\ \text{cm}
    yy(11.09±0.01) cm(11.09 \pm 0.01)\ \text{cm}
    zz(1.62±0.01) cm(1.62 \pm 0.01)\ \text{cm}

    In (b)(i) the density of the glass is determined from these measurements.

    The true value of the density of the glass is different from the answer in (b)(i) because of a systematic error in the measurements.

    Suggest one possible cause of this systematic error.

    Fig. 1.1 from the question paper: the glass block.

    Fig. 1.1 from the question paper: the glass block.

    Stuck? Show hint

    Density comes from mass ÷ volume — think what a wrongly-zeroed instrument would do to either.

    Show solution
    1. 1

      Any instrument reading too high (or too low) by a fixed amount produces exactly this pattern. One sufficient answer: the balance used for the mass had a zero error, reading a small mass before the block was placed on it.

      A zero error shifts every mass reading by the same amount, shifting the calculated density the same way every time.

    2. 2

      Equally acceptable: calipers measuring the block's dimensions with a zero error, or any wrongly-calibrated instrument (e.g. a balance reading consistently high against a known mass).

    Answer

    A zero error on the balance (or calipers), or a wrongly-calibrated instrument — any fixed offset applied to every reading.

  4. 4

    A top-pan balance always reads 0.4 g0.4\ \text{g} too high. A student weighs one object ten times and averages. State and explain the effect of the fault on (a) the accuracy of the mean, (b) the precision of the readings.

    Stuck? Show hint

    Ask what the fault does to the whole set of readings, and what it leaves alone.

    Show solution
    1. 1

      (a) Every reading is inflated by the same 0.4 g0.4\ \text{g}, so the mean is also 0.4 g0.4\ \text{g} too high: the result is inaccurate.

      A fixed offset passes straight through averaging — this is precisely why repetition cannot cure a systematic error.

    2. 2

      (b) The fault adds the same amount to every reading, so differences between readings are unchanged: the scatter stays as it was, so the precision is unaffected — the readings keep the same spread, just around a value 0.4 g0.4\ \text{g} too high.

      Precision depends only on how the readings differ from each other, and a fixed offset does not change any difference.

    Answer

    (a) The mean is 0.4 g0.4\ \text{g} too high — inaccurate. (b) Scatter unchanged — still precise.

06

Uncertainty in a derived quantity

Syllabus requirement · §1.3

“

assess the uncertainty in a derived quantity by simple addition of absolute or percentage uncertainties

”

A result without an uncertainty is incomplete

Almost no quantity in physics is measured directly: density comes from a mass and three lengths, resistance from a voltmeter reading and an ammeter reading. Each measured input carries an uncertainty, and the calculated result inherits one. This section gives the rules for working out how big that inherited uncertainty is. You need it to decide whether two results agree with each other, or with an accepted value.

Three ways to quote the same uncertainty

Take a length quoted as x=25.6 cm±0.4 cmx = 25.6\ \text{cm} \pm 0.4\ \text{cm}.

  • Absolute uncertainty Δx=0.4 cm\Delta x = 0.4\ \text{cm} — same units as the value itself. For a single reading it is usually taken as half the resolution (smallest scale division) of the instrument; for repeat readings, half the range of the repeats.
  • Fractional uncertainty Δxx=0.425.6=0.016\dfrac{\Delta x}{x} = \dfrac{0.4}{25.6} = 0.016 (about 1/641/64 of the value).
  • Percentage uncertainty =Δxx×100=1.6%= \dfrac{\Delta x}{x} \times 100 = 1.6\%.

All three carry exactly the same information; the combining rules below simply work more naturally in one form or the other.

Where the rules come from: worst-case reasoning

Rather than memorising rules, derive them once with invented numbers — then you can always rebuild them.

Rule for sums and differences: add absolute uncertainties. Suppose a=100±1a = 100 \pm 1 and b=50±1b = 50 \pm 1, so y=a+b=150y = a + b = 150. In the worst case, aa and bb are both high at once:

ymax=101+51=152y_{\text{max}} = 101 + 51 = 152

That is 150+2150 + 2: the uncertainty of the sum is Δy=1+1=2=Δa+Δb\Delta y = 1 + 1 = 2 = \Delta a + \Delta b. The worst case on the low side (99+49=14899 + 49 = 148) agrees. Subtraction behaves identically (y=a−b=50y = a - b = 50 has worst cases 101−49=52101 - 49 = 52 and 99−51=4899 - 51 = 48: again ±2\pm 2), because subtracting a too-low bb inflates the result just as much.

Rule for products and quotients: add percentage uncertainties. Take a=100±1%a = 100 \pm 1\% and b=50±2%b = 50 \pm 2\%, so y=ab=5000y = ab = 5000. Worst case high:

ymax=101×51=5151y_{\text{max}} = 101 \times 51 = 5151

That is 151151 above 50005000, i.e. 1515000≈3%=1%+2%\frac{151}{5000} \approx 3\% = 1\% + 2\%. The worst case low (99×49=485199 \times 49 = 4851, about 3%3\% down) agrees. So

Δyy=Δaa+Δbb\frac{\Delta y}{y} = \frac{\Delta a}{a} + \frac{\Delta b}{b}

A quotient works the same way: dividing by a number whose value might be 2%2\% low costs the same as multiplying by one 2%2\% high.

Rule for powers: multiply by the power. If y=a2y = a^2, then y=a×ay = a \times a, and the product rule adds the same percentage uncertainty to itself: 2×Δa/a2 \times \Delta a/a. In general y=any = a^n gives n×Δa/an \times \Delta a / a. A squared quantity's fractional uncertainty counts twice, a cubed one's three times.

Constants carry nothing. A number like 22 or π\pi is exact — it contributes zero uncertainty. So if y=a/2y = a/2, the percentage uncertainty of yy equals that of aa, and the absolute uncertainty is halved along with the value: a=8.0±0.4a = 8.0 \pm 0.4 gives y=4.0±0.2y = 4.0 \pm 0.2.

The combining rules
y=a+b or y=a−b:Δy=Δa+Δby = a + b \ \text{or}\ y = a - b:\quad \Delta y = \Delta a + \Delta b

Sum or difference → add ABSOLUTE uncertainties

y=ab or y=ab:Δyy=Δaa+Δbby = ab \ \text{or}\ y = \tfrac{a}{b}:\quad \frac{\Delta y}{y} = \frac{\Delta a}{a} + \frac{\Delta b}{b}

Product or quotient → add PERCENTAGE (fractional) uncertainties

y=an:Δyy=n Δaay = a^n:\quad \frac{\Delta y}{y} = n\,\frac{\Delta a}{a}

Power n → multiply the percentage uncertainty by n

constants (2,π): no uncertainty\text{constants } (2, \pi)\text{: no uncertainty}

Pure numbers contribute nothing

Converting back, and rounding

Once the percentage uncertainty of the result is known, convert back to absolute form when asked:

Δy=percentage uncertainty100×y\Delta y = \frac{\text{percentage uncertainty}}{100} \times y

Then round using two rules:

  • quote the uncertainty to 1 significant figure (at most 2);
  • make the last significant figure of the value match the uncertainty: 46±3.746 \pm 3.7 becomes 46±446 \pm 4, never 45.8±3.745.8 \pm 3.7.

Do two results agree? Turn each into a range: 5.0±0.35.0 \pm 0.3 runs from 4.74.7 to 5.35.3, and 5.6±0.45.6 \pm 0.4 runs from 5.25.2 to 6.06.0. The ranges overlap (between 5.25.2 and 5.35.3), so the two results could be the same quantity. If the ranges do not overlap, the results disagree.

Uncertainty in any calculated quantity
  1. 1

    Write the equation the quantity is calculated from.

  2. 2

    Label each measured quantity with its percentage uncertainty (convert from absolute if necessary).

  3. 3

    Add the percentages, first multiplying by any power each quantity is raised to. Constants contribute nothing.

  4. 4

    Convert back to absolute if asked: multiply the total percentage by the calculated value, then round to 1 s.f.

    The question says "absolute uncertainty" — do not stop at the percentage.

A clean demonstration

Given x=4.0±2%x = 4.0 \pm 2\% and y=2.0±3%y = 2.0 \pm 3\%, find z=xy2z = xy^2 with its absolute uncertainty.

Value: z=4.0×2.02=4.0×4.0=16z = 4.0 \times 2.0^2 = 4.0 \times 4.0 = 16

Percentage uncertainty, piece by piece: xx enters once, carrying 2%2\%; yy is squared, so its 3%3\% counts twice:

Δzz=2%+(2×3%)=8%\frac{\Delta z}{z} = 2\% + (2 \times 3\%) = 8\%

Convert back: Δz=8100×16=1.28→±1  (1 s.f.)\Delta z = \frac{8}{100} \times 16 = 1.28 \rightarrow \pm 1 \ \ (\text{1 s.f.})

So z=16±1z = 16 \pm 1. Notice how every rule appeared once: product (add percentages), power (double the yy contribution), constant-free arithmetic, then round.

Combining three percentage uncertainties with a square

9702/22 O/N 2025 Q1(c)

A quantity cc relating to the motion of the balloon is calculated from three measured quantities kk, FF and vv using the formula

c=2kFv2c = \frac{2kF}{v^2}

The percentage uncertainties in the measured quantities are given in Table 1.2.

measured quantitypercentage uncertainty
kk5%5\%
FF3%3\%
vv4%4\%

The calculated value of cc is 1.81.8.

Determine the absolute uncertainty in cc.

Show full working
  1. 1

    Deal with the constant first: the 22 in the numerator is exact and contributes no uncertainty.

    Clearing constants out of the way stops them being counted later — a common slip.

  2. 2

    vv is squared, so its percentage uncertainty counts twice: v2 contributes 2×4%=8%v^2 \text{ contributes } 2 \times 4\% = 8\%

    This doubling is the step most easily forgotten — the square applies to the uncertainty as well as to the value. The mark scheme's first mark is for 5 + 3 + (2 × 4).

  3. 3

    Add the three contributions: Δcc=5%+3%+8%=16%\frac{\Delta c}{c} = 5\% + 3\% + 8\% = 16\%

  4. 4

    Convert back to absolute: identify the pieces — total percentage =16= 16, value c=1.8c = 1.8 — then substitute:

    Δc=16100×1.8=0.288\Delta c = \frac{16}{100} \times 1.8 = 0.288
  5. 5

    Round to 1 significant figure and match the value to it: c=1.8±0.3c = 1.8 \pm 0.3

    0.288 becomes 0.3, and the value stays at 1.8 — one decimal place, matching the uncertainty's.

Answer

Δc=±0.3\Delta c = \pm 0.3 (from a total percentage uncertainty of 16%16\%), giving c=1.8±0.3c = 1.8 \pm 0.3.

Write each variable's contribution on its own line before adding — squares doubled, constants skipped.

Resistivity: four measurements and a squared diameter

9702/24 O/N 2025 Q5(b)(iii)

A student uses a circuit containing an ammeter, a voltmeter and a cell to take measurements to determine the resistance of a length of nichrome wire.

The student also measures the length and the diameter of the wire. Table 5.1 shows the measurements recorded for each quantity.

quantitymeasurement
length(0.864±0.001) m(0.864 \pm 0.001)\ \text{m}
diameter(0.496±0.002) mm(0.496 \pm 0.002)\ \text{mm}
voltmeter reading(1.38±0.02) V(1.38 \pm 0.02)\ \text{V}
ammeter reading(0.276±0.001) A(0.276 \pm 0.001)\ \text{A}

In earlier parts the resistance R=V/IR = V/I and the resistivity ρ=RA/L\rho = RA/L of the nichrome are calculated, where A=πd2/4A = \pi d^2/4 is the cross-sectional area; together these give ρ=πVd24IL\rho = \dfrac{\pi V d^2}{4 I L}.

Calculate the percentage uncertainty in ρ\rho.

Show full working
  1. 1

    π\pi and 44 are exact constants — they contribute nothing.

  2. 2

    Fractional uncertainty in VV (enters once): 0.021.38=0.0145\frac{0.02}{1.38} = 0.0145

  3. 3

    Fractional uncertainty in dd: 0.0020.496=0.00403\frac{0.002}{0.496} = 0.00403 But dd is squared, so this counts twice: 2×0.00403=0.008062 \times 0.00403 = 0.00806

    The diameter enters squared — forgetting to double its fractional uncertainty is THE mark-dropper here.

  4. 4

    Fractional uncertainty in LL (enters once, on the bottom): 0.0010.864=0.00116\frac{0.001}{0.864} = 0.00116

  5. 5

    Fractional uncertainty in II (once, on the bottom): 0.0010.276=0.00362\frac{0.001}{0.276} = 0.00362

  6. 6

    Add all four contributions: 0.00116+0.00806+0.0145+0.00362=0.02730.00116 + 0.00806 + 0.0145 + 0.00362 = 0.0273

  7. 7

    Convert to a percentage: 0.0273×100=2.73%≈2.7%0.0273 \times 100 = 2.73\% \approx 2.7\%

Answer

Percentage uncertainty in ρ≈2.7%\rho \approx 2.7\%.

Division costs exactly what multiplication costs — quantities on the bottom of a fraction add their percentage uncertainties just the same.

Your turn

The first item is a difference, so it adds absolute uncertainties. The rest use the method above: equation → label percentages → add (doubling or cubing where powered) → convert back.

  1. 19702/14 M/J 2025 Q3

    Calipers are used to determine the thickness of the wall of a glass tube. The following measurements are made.

    internal diameter of the tube =(10.0±0.1) mm= (10.0 \pm 0.1)\ \text{mm}
    external diameter of the tube =(12.0±0.1) mm= (12.0 \pm 0.1)\ \text{mm}

    What is the thickness of the wall of the tube?

    Options

    A   (1.0±0.1) mm(1.0 \pm 0.1)\ \text{mm}
    B   (1.0±0.2) mm(1.0 \pm 0.2)\ \text{mm}
    C   (2.0±0.1) mm(2.0 \pm 0.1)\ \text{mm}
    D   (2.0±0.2) mm(2.0 \pm 0.2)\ \text{mm}

    Fig. 1 from the question paper: the glass tube.

    Fig. 1 from the question paper: the glass tube.

    Stuck? Show hint

    The difference of the diameters is the wall counted twice — once on each side of the tube.

    Show solution
    1. 1

      Difference of the diameters: 12.0−10.0=2.0 mm12.0 - 10.0 = 2.0\ \text{mm} This covers the wall on both sides of the tube.

      A diameter crosses the tube, passing through the wall twice. Forgetting this gives options C and D.

    2. 2

      Uncertainty of a difference: add the absolute uncertainties. Δ=0.1+0.1=0.2 mm\Delta = 0.1 + 0.1 = 0.2\ \text{mm} so the difference is (2.0±0.2) mm(2.0 \pm 0.2)\ \text{mm}.

      Subtracting never reduces uncertainty: in the worst case one diameter is high and the other low.

    3. 3

      Halve to get one wall. Dividing by the exact number 22 halves the value and its absolute uncertainty: t=2.02=1.0 mmΔt=0.22=0.1 mmt = \frac{2.0}{2} = 1.0\ \text{mm} \qquad \Delta t = \frac{0.2}{2} = 0.1\ \text{mm}

      The percentage uncertainty stays 10%, so the absolute uncertainty halves with the value. Keeping ±0.2 gives the trap answer B.

    4. 4

      So t=(1.0±0.1) mmt = (1.0 \pm 0.1)\ \text{mm} — option A.

    Answer

    A — (1.0±0.1) mm(1.0 \pm 0.1)\ \text{mm}.

  2. 29702/13 O/N 2025 Q2

    Two quantities are measured.

    L=6.8±0.1 cmL = 6.8 \pm 0.1\ \text{cm}

    T=2.42±0.08 sT = 2.42 \pm 0.08\ \text{s}

    LL and TT are related to XX by the equation shown.

    X=4π2LT2X = \frac{4\pi^2 L}{T^2}

    What is the calculated value and uncertainty of XX?

    Options

    A   45.8±0.2 cm s−245.8 \pm 0.2\ \text{cm s}^{-2}
    B   45.8±0.3 cm s−245.8 \pm 0.3\ \text{cm s}^{-2}
    C   46±2 cm s−246 \pm 2\ \text{cm s}^{-2}
    D   46±4 cm s−246 \pm 4\ \text{cm s}^{-2}

    Stuck? Show hint

    Convert both absolute uncertainties to percentages before combining — and remember TT is squared.

    Show solution
    1. 1

      Calculate the pieces of the value first: T2=2.422=5.8564 s24π2=39.48T^2 = 2.42^2 = 5.8564\ \text{s}^2 \qquad 4\pi^2 = 39.48

    2. 2

      Substitute and evaluate: X=39.48×6.85.8564=268.55.8564=45.8 cm s−2X = \frac{39.48 \times 6.8}{5.8564} = \frac{268.5}{5.8564} = 45.8\ \text{cm s}^{-2}

      Keep a spare figure (45.8) until the uncertainty is known — the final rounding depends on it.

    3. 3

      Percentage uncertainty in LL: 0.16.8×100=1.47%\frac{0.1}{6.8} \times 100 = 1.47\%

    4. 4

      Percentage uncertainty in TT: 0.082.42×100=3.31%\frac{0.08}{2.42} \times 100 = 3.31\% and since TT is squared this counts twice: 2×3.31%=6.61%2 \times 3.31\% = 6.61\%.

    5. 5

      Add: ΔXX=1.47%+6.61%=8.08%\frac{\Delta X}{X} = 1.47\% + 6.61\% = 8.08\%

    6. 6

      Convert back to absolute: ΔX=8.08100×45.8=3.70→±4  (1 s.f.)\Delta X = \frac{8.08}{100} \times 45.8 = 3.70 \rightarrow \pm 4\ \ (\text{1 s.f.})

    7. 7

      Round the value to match: X=46±4 cm s−2X = 46 \pm 4\ \text{cm s}^{-2} — option D.

      A and B keep 45.8 with far too small an uncertainty; C forgets to double the uncertainty in T for the square.

    Answer

    D — X=46±4 cm s−2X = 46 \pm 4\ \text{cm s}^{-2}

  3. 39702/22 F/M 2025 Q1(b)(ii)

    Two solid cubes, A and B, are measured to determine the density of their materials.

    Table 1.1 shows the measurements for cube A.

    quantitymeasurement
    length of side(1.53±0.01) cm(1.53 \pm 0.01)\ \text{cm}
    mass(31.3±0.5) g(31.3 \pm 0.5)\ \text{g}

    Calculate the percentage uncertainty in the density of the material of cube A.

    Stuck? Show hint

    Density = mass ÷ volume, and the volume of a cube of side LL is L3L^3.

    Show solution
    1. 1

      Write the equation: ρ=mV=mL3\rho = \frac{m}{V} = \frac{m}{L^3} so the mass enters once and the side length is cubed.

    2. 2

      Percentage uncertainty in the mass: 0.531.3×100=1.60%\frac{0.5}{31.3} \times 100 = 1.60\%

    3. 3

      Percentage uncertainty in the side length: 0.011.53×100=0.654%\frac{0.01}{1.53} \times 100 = 0.654\% The side is cubed (L3L^3), so this counts three times: 3×0.654%=1.96%3 \times 0.654\% = 1.96\%.

      Cubed, not squared — count the exponent carefully before multiplying.

    4. 4

      Add: Δρρ=1.60%+1.96%=3.56%≈4%\frac{\Delta\rho}{\rho} = 1.60\% + 1.96\% = 3.56\% \approx 4\%

      The mark scheme quotes 4% — uncertainties are conventionally given to 1 significant figure, so round the 3.56% at the end rather than part-way through.

    Answer

    4%4\% (1.60%+3×0.654%=3.56%1.60\% + 3 \times 0.654\% = 3.56\%, quoted as 4%4\%).

  4. 49702/22 F/M 2025 Q1(b)(iii)

    (Continuing the previous question: the calculated density of the material of cube A is 8.7×103 kg m−38.7 \times 10^{3}\ \text{kg m}^{-3}, with the percentage uncertainty of 4%4\% found above.)

    The density of the material of cube B is determined to be 9.2×103 kg m−3±6%9.2 \times 10^{3}\ \text{kg m}^{-3} \pm 6\%.

    State and explain whether cube A and cube B could be made from the same material.

    Stuck? Show hint

    Work out the range each density could span, then look for overlap.

    Show solution
    1. 1

      Range of cube A: 4%4\% of 8.7×1038.7 \times 10^{3} is 0.35×1030.35 \times 10^{3}, so

      A=(8.7±0.35)×103 kg m−3:8.35→9.05×103A = (8.7 \pm 0.35) \times 10^{3}\ \text{kg m}^{-3}: \quad 8.35 \rightarrow 9.05 \times 10^{3}
    2. 2

      Range of cube B: 6%6\% of 9.2×1039.2 \times 10^{3} is 0.55×1030.55 \times 10^{3}, so

      B=(9.2±0.55)×103 kg m−3:8.65→9.75×103B = (9.2 \pm 0.55) \times 10^{3}\ \text{kg m}^{-3}: \quad 8.65 \rightarrow 9.75 \times 10^{3}
    3. 3

      Compare ranges: A reaches up to 9.059.05 and B reaches down to 8.658.65, so they overlap between 8.658.65 and 9.05×103 kg m−39.05 \times 10^{3}\ \text{kg m}^{-3}.

      Overlap is precisely the criterion: within their uncertainties the two results agree, so the same metal is possible.

    4. 4

      Therefore yes — the two cubes could be made of the same material, because their ranges of possible density overlap.

    Answer

    Yes — A spans 8.358.35–9.059.05 and B spans 8.658.65–9.759.75 (both ×103 kg m−3\times 10^{3}\ \text{kg m}^{-3}); the ranges overlap, so the densities agree within uncertainty.

  5. 59702/12 O/N 2025 Q4

    A ball is released from rest. The distance the ball falls and the time the ball takes to fall that distance are both measured.

    The percentage uncertainty in the measured distance is negligible. The percentage uncertainty in the measured time is 4%4\%.

    The distance and the time are then used to calculate the acceleration of free fall.

    Air resistance is negligible.

    What is the percentage uncertainty in the calculated value of the acceleration of free fall?

    Options

    A   2%2\%
    B   4%4\%
    C   8%8\%
    D   16%16\%

    Stuck? Show hint

    For an object falling from rest, s=12gt2s = \tfrac{1}{2}gt^2 (an equation of motion from the AS Kinematics note).

    Show solution
    1. 1

      Find the equation first. For a fall from rest, s=12gt2s = \tfrac{1}{2}gt^2, so rearranging for gg: g=2st2g = \frac{2s}{t^2}

      The question does not give the equation — you must supply it. You meet it properly in the AS Kinematics note; here you only need to see that t is squared.

    2. 2

      The 22 is an exact constant and the uncertainty in ss is stated negligible — both contribute nothing.

    3. 3

      tt is squared, so its 4%4\% counts twice: Δgg=2×4%=8%\frac{\Delta g}{g} = 2 \times 4\% = 8\% — option C.

    Answer

    C — 8%8\%

  6. 69702/14 O/N 2025 Q3

    A stone is released from rest and falls vertically to the ground.

    The time taken to fall to the ground and the distance travelled are measured. The measurements are used to determine the acceleration of free fall.

    The percentage uncertainty in the measured time is 0.05%0.05\%. The percentage uncertainty in the measured distance fallen is 0.6%0.6\%.

    What is the percentage uncertainty in the calculated value of the acceleration of free fall?

    Options

    A   0.5%0.5\%
    B   0.7%0.7\%
    C   1.1%1.1\%
    D   1.3%1.3\%

    Show solution
    1. 1

      Same equation as the previous question: from rest, s=12gt2s = \tfrac{1}{2}gt^2, so g=2st2g = \frac{2s}{t^2}

    2. 2

      ss enters once, carrying 0.6%0.6\%.

    3. 3

      tt is squared, so its 0.05%0.05\% counts twice: 2×0.05%=0.10%2 \times 0.05\% = 0.10\%.

    4. 4

      Add: Δgg=0.6%+0.10%=0.7%\frac{\Delta g}{g} = 0.6\% + 0.10\% = 0.7\% — option B.

    Answer

    B — 0.7%0.7\%

07

Scalars and vectors; adding vectors

Syllabus requirement · §1.4

“

understand the difference between scalar and vector quantities and give examples of scalar and vector quantities included in the syllabus; add and subtract coplanar vectors

”

Direction changes everything

A scalar is a quantity with a magnitude and a unit — and nothing more. A vector is a quantity with a magnitude, a unit and a direction. That one extra piece of information changes how the quantity combines: two 6 N6\ \text{N} forces pointing the same way make a 12 N12\ \text{N} resultant (the resultant is the single vector with the same effect as the two together), but pointing opposite ways they make zero. Every mechanics topic that follows uses vectors.

Scalars (magnitude + unit)

Vectors (magnitude + unit + direction)

distance

displacement

speed

velocity

mass, time, temperature

acceleration

energy, charge

force

pressure, density

momentum

wavelength, potential difference

—

Learn both columns. Every vector's "magnitude only" cousin is a scalar (distance ↔ displacement, speed ↔ velocity) — but many scalars (energy, charge, temperature) have no vector partner at all.

The two classic classification traps

Energy and charge are scalars, even though they feel directional in use — a charge "flows" one way, energy is "transferred" somewhere, but neither quantity itself carries a direction. And speed is a scalar while velocity is a vector: a car going round a roundabout at a steady 20 m s−120\ \text{m s}^{-1} has constant speed but constantly changing velocity, because its direction changes. Note also that scalars and vectors both have a magnitude and a unit — the presence of a direction is the only difference.

Adding coplanar vectors: head-to-tail

Vectors in the same plane add by the head-to-tail construction:

  1. Draw the first vector a⃗\vec{a} to scale, in its own direction.
  2. From the head (arrow end) of a⃗\vec{a}, draw the second vector b⃗\vec{b} to scale, in its direction.
  3. The resultant runs from the tail of a⃗\vec{a} to the head of b⃗\vec{b}.

The order does not matter (a⃗+b⃗=b⃗+a⃗\vec{a} + \vec{b} = \vec{b} + \vec{a}) — either order closes the same triangle.

abR = a + bhead of a = tail of b

Head-to-tail addition: draw a, then b from a's head; the resultant runs from a's tail to b's head, closing the triangle.

Two vectors and an angle: the cosine rule

Place the two vectors tail-to-tail with the angle θ\theta between them, then slide BB along so its tail sits on the head of AA, completing the head-to-tail triangle. At that corner, BB still makes the angle θ\theta with the line of AA carried on, so the triangle's inside angle between sides AA and BB is 180∘−θ180^\circ - \theta (angles on a straight line add to 180∘180^\circ). The ordinary cosine rule for sides AA, BB with included angle CC is

R2=A2+B2−2ABcos⁡CR^2 = A^2 + B^2 - 2AB\cos C

Here C=180∘−θC = 180^\circ - \theta, so

R2=A2+B2−2ABcos⁡(180∘−θ)R^2 = A^2 + B^2 - 2AB\cos(180^\circ - \theta)

and since cos⁡(180∘−θ)=−cos⁡θ\cos(180^\circ - \theta) = -\cos\theta:

R2=A2+B2+2ABcos⁡θR^2 = A^2 + B^2 + 2AB\cos\theta

Special cases worth knowing on sight:

  • θ=0∘\theta = 0^\circ (same direction): cos⁡0=1\cos 0 = 1, so R=A+BR = A + B — plain addition.
  • θ=90∘\theta = 90^\circ: cos⁡90∘=0\cos 90^\circ = 0, so R=A2+B2R = \sqrt{A^2 + B^2} — Pythagoras.
  • equal vectors at θ=60∘\theta = 60^\circ: R2=A2+A2+2A2(0.5)=3A2R^2 = A^2 + A^2 + 2A^2(0.5) = 3A^2, so R=3 AR = \sqrt{3}\,A.
  • equal vectors at θ=120∘\theta = 120^\circ: R2=A2+A2+2A2(−0.5)=A2R^2 = A^2 + A^2 + 2A^2(-0.5) = A^2, so R=AR = A.
ABBRθθ180° − θR² = A² + B² + 2AB cos θ

A and B drawn tail-to-tail with angle θ between them; B slid to the head of A closes the triangle. The inside angle at that corner is 180° − θ, which turns the cosine rule's minus sign into the plus sign of R² = A² + B² + 2AB cos θ.

Subtracting vectors: add the reverse

a⃗−b⃗=a⃗+(−b⃗)\vec{a} - \vec{b} = \vec{a} + (-\vec{b})

Reversing a vector flips its direction while keeping its magnitude, so subtraction becomes another head-to-tail addition — with b⃗\vec{b}'s arrow turned round.

The most common use is a change in a vector quantity: change = final − initial. For a velocity that changes from u⃗\vec{u} to v⃗\vec{v}, the change in velocity is Δv⃗=v⃗−u⃗=v⃗+(−u⃗)\Delta\vec{v} = \vec{v} - \vec{u} = \vec{v} + (-\vec{u}).

ba−ba − bsubtracting b = adding a vector of the same lengthin the opposite direction

Subtraction as addition of the reversed vector: a − b is drawn by flipping b end-for-end and adding it head-to-tail to a.

A clean demonstration

Addition at 90∘90^\circ. Two forces act at a point: 5.0 N5.0\ \text{N} east and 12.0 N12.0\ \text{N} north. Perpendicular vectors, so θ=90∘\theta = 90^\circ and the cosine rule collapses to Pythagoras:

R=5.02+12.02=25+144=169=13 NR = \sqrt{5.0^2 + 12.0^2} = \sqrt{25 + 144} = \sqrt{169} = 13\ \text{N}

Subtraction. Let a⃗=8.0 N\vec{a} = 8.0\ \text{N} east and b⃗=3.0 N\vec{b} = 3.0\ \text{N} east. Then a⃗−b⃗\vec{a} - \vec{b} means a⃗\vec{a} plus 3.0 N3.0\ \text{N} west:

a⃗−b⃗=8.0 N east+3.0 N west=5.0 N east\vec{a} - \vec{b} = 8.0\ \text{N east} + 3.0\ \text{N west} = 5.0\ \text{N east}

If instead b⃗=3.0 N\vec{b} = 3.0\ \text{N} west, then a⃗−b⃗=8.0 N\vec{a} - \vec{b} = 8.0\ \text{N} east + 3.0 N+\ 3.0\ \text{N} east =11.0 N= 11.0\ \text{N} east. Same subtraction, opposite result — the direction of the vector being subtracted matters at every stage.

Resultant of two equal forces at 60°

9702/13 O/N 2025 Q4

The diagram shows two forces of 6.0 N6.0\ \text{N} acting on an object. The angle between the lines of action of the two forces is 60∘60^\circ.

What is the magnitude of the resultant force?

Options

A   6.0 N6.0\ \text{N}
B   7.9 N7.9\ \text{N}
C   10 N10\ \text{N}
D   12 N12\ \text{N}

Fig. 1 from the question paper.

Fig. 1 from the question paper.

Show full working
  1. 1

    Two vectors with a stated angle between them → cosine rule form:

    R2=A2+B2+2ABcos⁡θR^2 = A^2 + B^2 + 2AB\cos\theta

    Identify the pieces: A=6.0 NA = 6.0\ \text{N}, B=6.0 NB = 6.0\ \text{N}, θ=60∘\theta = 60^\circ.

    The angle between the vectors is used exactly as given — the 180° − θ conversion is already built into the formula, so do not apply it again.

  2. 2

    Substitute each piece: R2=6.02+6.02+2(6.0)(6.0)cos⁡60∘R^2 = 6.0^2 + 6.0^2 + 2(6.0)(6.0)\cos 60^\circ

  3. 3

    Evaluate term by term: 6.02=366.0^2 = 36 and 6.02=366.0^2 = 36; cos⁡60∘=0.5\cos 60^\circ = 0.5, so the cross term is 2×6.0×6.0×0.5=362 \times 6.0 \times 6.0 \times 0.5 = 36:

    R2=36+36+36=108R^2 = 36 + 36 + 36 = 108
  4. 4

    Take the square root: R=108=10.4 N≈10 NR = \sqrt{108} = 10.4\ \text{N} \approx 10\ \text{N} — option C.

    The tempting wrong answer 12 N (option D) comes from just adding the magnitudes, which is only valid when the vectors point the same way (θ = 0). And 6.0 N (option A) would be the resultant if the angle were 120° rather than 60° — equal vectors at 120° give R = A. The angle of 60° must shrink the answer below 12 but keep it well above 6 — 10 N is exactly that.

Answer

C — 10 N10\ \text{N} (R2=36+36+36=108R^2 = 36 + 36 + 36 = 108, so R≈10 NR \approx 10\ \text{N}).

For any two vectors, the resultant always lies between |A − B| and A + B — use that to sanity-check any option list.

Your turn

  1. 19702/22 M/J 2025 Q1(a)

    Table 1.1 lists some physical quantities. Identify with ticks (✓) which quantities are vectors and which are scalars.

    quantityscalarvector
    acceleration
    displacement
    gravitational potential energy
    speed
    temperature
    Show solution
    1. 1

      Acceleration — a rate of change of velocity, which carries a direction: V.

    2. 2

      Displacement — distance in a stated direction: V.

    3. 3

      Gravitational potential energy — energy is a scalar, whatever its origin: S.

      The energy trap from the callout: it feels directional but carries no direction of its own.

    4. 4

      Speed — the magnitude-only cousin of velocity: S.

    5. 5

      Temperature — no direction attaches to it: S.

    Answer

    acceleration V; displacement V; gravitational potential energy S; speed S; temperature S.

  2. 29702/23 M/J 2021 Q1(a)(ii)

    A property of a vector quantity, that is not a property of a scalar quantity, is direction. For example, velocity has direction but speed does not.

    State two properties that are possessed by both scalar and vector physical quantities.

    Show solution
    1. 1

      Both have a magnitude (a number).

    2. 2

      Both have a unit.

      The question deliberately asks for what is shared, not what differs — direction belongs to vectors only, so it must not appear in the answer.

    Answer

    A magnitude and a unit.

  3. 39702/22 O/N 2024 Q1(a)

    State what is meant by a vector quantity.

    Show solution
    1. 1

      A vector quantity has both magnitude and direction (and, like every physical quantity, a unit).

    Answer

    A quantity with both magnitude and direction.

  4. 4

    A rower rows at 3.0 m s−13.0\ \text{m s}^{-1} relative to the water, aiming straight across a river. The water itself flows parallel to the bank at 4.0 m s−14.0\ \text{m s}^{-1}. Find the magnitude of the rower's resultant velocity and the angle it makes with the rower's intended direction.

    Stuck? Show hint

    The two velocities are perpendicular — which special case of the cosine rule applies?

    Show solution
    1. 1

      The two velocities are perpendicular (θ=90∘\theta = 90^\circ), so cos⁡90∘=0\cos 90^\circ = 0 and the cosine rule reduces to Pythagoras: R=A2+B2R = \sqrt{A^2 + B^2}

      Both are velocities in m s⁻¹, so they can be combined; the right angle is what allows Pythagoras.

    2. 2

      Identify the pieces, A=3.0 m s−1A = 3.0\ \text{m s}^{-1} and B=4.0 m s−1B = 4.0\ \text{m s}^{-1}, and substitute: R=3.02+4.02=9+16=25=5.0 m s−1R = \sqrt{3.0^2 + 4.0^2} = \sqrt{9 + 16} = \sqrt{25} = 5.0\ \text{m s}^{-1}

    3. 3

      Direction: the component along the bank (4.04.0) is perpendicular to the intended direction, so the angle θ\theta between the resultant and the intended (straight-across) direction satisfies

      tan⁡θ=4.03.0⟹θ=53∘\tan\theta = \frac{4.0}{3.0} \quad\Longrightarrow\quad \theta = 53^\circ

      The resultant is dragged 53° away from where the rower is aiming — which is why aiming straight across a flowing river never gets you straight across.

    Answer

    5.0 m s−15.0\ \text{m s}^{-1}, at 53∘53^\circ from the intended direction (i.e. 37∘37^\circ to the bank).

  5. 59702/11 M/J 2024 Q3

    The velocity of an object changes from an initial velocity uu to a final velocity vv. The vectors represent these velocities.

    Which single vector represents the change in velocity of the object?

    Fig. 1: the initial velocity u and the final velocity v.

    Fig. 1: the initial velocity u and the final velocity v.

    Options A to D.

    Options A to D.

    Stuck? Show hint

    Change = final − initial, and subtracting uu means adding uu turned round.

    Show solution
    1. 1

      Write the change: Δv⃗=v⃗−u⃗=v⃗+(−u⃗)\Delta\vec{v} = \vec{v} - \vec{u} = \vec{v} + (-\vec{u})

      Final minus initial. Doing u − v instead gives the reversed arrow, which is option A.

    2. 2

      Read the directions from Fig. 1: u⃗\vec{u} points to the right, v⃗\vec{v} points straight down. So −u⃗-\vec{u} points to the left.

    3. 3

      Add head-to-tail: draw v⃗\vec{v} (down), then from its head draw −u⃗-\vec{u} (left). The resultant runs from the start of v⃗\vec{v} to the end of −u⃗-\vec{u}: it points down and to the left.

    4. 4

      Only option C points down and to the left.

      B points down-right (that is v + u, an addition). D points up-left and A up-right: each has at least one direction backwards.

    Answer

    C — the arrow pointing down and to the left (v⃗+(−u⃗)\vec{v} + (-\vec{u})).

08

Resolving into perpendicular components

Syllabus requirement · §1.4

“

represent a vector as two perpendicular components

”

Why resolve? Because perpendicular directions are independent

Addition combines two vectors into one. Resolution runs the film backwards: it splits one vector into two perpendicular components that add back to it. Why do this? Motion or forces along perpendicular directions do not affect each other, so one awkward 2-D problem becomes two easy 1-D problems. Horizontal and vertical, or along a slope and perpendicular to it: the mechanics topics that follow use this all the time.

Where cos and sin come from

Draw the vector FF at angle θ\theta to the xx-direction and drop a perpendicular from its head onto the xx-axis. The vector is the hypotenuse of a right-angled triangle whose two legs are the components: FxF_x along xx (adjacent to θ\theta) and FyF_y perpendicular to xx (opposite θ\theta). Right-angle trigonometry says

cos⁡θ=adjacenthypotenuse=FxFsin⁡θ=oppositehypotenuse=FyF\cos\theta = \frac{\text{adjacent}}{\text{hypotenuse}} = \frac{F_x}{F} \qquad\qquad \sin\theta = \frac{\text{opposite}}{\text{hypotenuse}} = \frac{F_y}{F}

Multiplying both sides of each equation by FF:

Fx=Fcos⁡θFy=Fsin⁡θF_x = F\cos\theta \qquad\qquad F_y = F\sin\theta

The cos goes with the adjacent side — the component along the direction you measured θ\theta from. A two-second check that never fails: put θ=0\theta = 0. The vector then points entirely along xx, and indeed Fx=Fcos⁡0=FF_x = F\cos 0 = F while Fy=Fsin⁡0=0F_y = F\sin 0 = 0. Any cos/sin assignment that fails this check is backwards.

FF cos θ (= Fx)F sin θ (= Fy)θcos goes with the adjacent side, sin with the opposite

Resolving F at angle θ to the x-direction: the adjacent leg is F cos θ, the opposite leg is F sin θ. The check θ = 0 (all of F along x) confirms which trig function goes where.

Recombining components

Given the components, the original vector is recovered by adding them head-to-tail. They are perpendicular, so Pythagoras applies (the θ=90∘\theta = 90^\circ case in “Scalars and vectors; adding vectors”):

R=Rx2+Ry2tan⁡θ=RyRxR = \sqrt{R_x^2 + R_y^2} \qquad\qquad \tan\theta = \frac{R_y}{R_x}

The magnitude comes from Pythagoras and the direction from the tangent — the angle measured from the same axis the components were taken along. A good habit: recombine at the end of a long calculation to confirm you land back on the original vector.

RxRyRθR = √(Rx² + Ry²)tan θ = Ry / Rx

Recombining: components Rx and Ry rebuild a resultant of magnitude √(Rx² + Ry²) at angle tan⁻¹(Ry/Rx) to the x-direction.

Resolving any vector
  1. 1

    Sketch the vector at its angle, roughly to scale.

  2. 2

    Mark θ\theta from a defined axis — say explicitly which direction you measured the angle from.

    cos and sin swap depending on which axis θ is measured from; pinning the axis down prevents the swap.

  3. 3

    Adjacent side gets cos, opposite side gets sin, relative to that angle.

  4. 4

    Sanity-check with θ=0\theta = 0 or 90∘90^\circ: at 0∘0^\circ everything lies along the axis, at 90∘90^\circ nothing does.

    Two seconds of checking catches a cos/sin swap, the most common slip when resolving.

A clean demonstration

A ball is thrown with speed 20 m s−120\ \text{m s}^{-1} at 30∘30^\circ above the horizontal. Resolve it.

Horizontal component — adjacent to the 30∘30^\circ angle, so cos:

vx=vcos⁡θ=20×cos⁡30∘=20×0.866=17.3 m s−1≈17 m s−1v_x = v\cos\theta = 20 \times \cos 30^\circ = 20 \times 0.866 = 17.3\ \text{m s}^{-1} \approx 17\ \text{m s}^{-1}

Vertical component — opposite the angle, so sin:

vy=vsin⁡θ=20×sin⁡30∘=20×0.5=10 m s−1v_y = v\sin\theta = 20 \times \sin 30^\circ = 20 \times 0.5 = 10\ \text{m s}^{-1}

Sanity check. 30∘30^\circ is closer to 0∘0^\circ than to 90∘90^\circ, so the horizontal component should be the larger — and 17>1017 > 10 ✓.

Recombine to close the loop:

R=17.32+102=299.3+100=399.3≈20 m s−1✓R = \sqrt{17.3^2 + 10^2} = \sqrt{299.3 + 100} = \sqrt{399.3} \approx 20\ \text{m s}^{-1} ✓

Components of a kicked ball's velocity

9702/24 O/N 2025 Q1(a)(i)

A child kicks a ball so that it leaves horizontal ground with a velocity of 28 m s−128\ \text{m s}^{-1} at an angle of 34∘34^\circ to the horizontal, as shown in Fig. 1.1.

Air resistance is negligible. The ball leaves the ground at time t=0t = 0.

Calculate the horizontal component vHv_{\text{H}} and the vertical component vVv_{\text{V}} of the velocity of the ball immediately after it has left the ground.

Fig. 1.1 from the question paper.

Fig. 1.1 from the question paper.

Show full working
  1. 1

    The angle 34∘34^\circ is measured from the horizontal, so the horizontal component is the adjacent one and takes cos:

    vH=vcos⁡θ=28×cos⁡34∘v_{\text{H}} = v\cos\theta = 28 \times \cos 34^\circ

    Say which axis the angle is from before choosing cos or sin — that single sentence prevents the swap.

  2. 2

    Evaluate: vH=28×0.829=23.2 m s−1≈23 m s−1v_{\text{H}} = 28 \times 0.829 = 23.2\ \text{m s}^{-1} \approx 23\ \text{m s}^{-1} (2 s.f., matching the data).

  3. 3

    The vertical component is the opposite one, so sin:

    vV=vsin⁡θ=28×sin⁡34∘v_{\text{V}} = v\sin\theta = 28 \times \sin 34^\circ
  4. 4

    Evaluate: vV=28×0.559=15.7 m s−1≈16 m s−1v_{\text{V}} = 28 \times 0.559 = 15.7\ \text{m s}^{-1} \approx 16\ \text{m s}^{-1}

  5. 5

    Sanity check: 34∘34^\circ is less than 45∘45^\circ, so the horizontal component should dominate — 23>1623 > 16 ✓.

    Quoting 23 and 16 (not 23.2 and 15.7) is deliberate: the inputs have 2 s.f., so the answers must too.

Answer

vH=23 m s−1v_{\text{H}} = 23\ \text{m s}^{-1}, vV=16 m s−1v_{\text{V}} = 16\ \text{m s}^{-1}.

Angle from the horizontal → horizontal takes cos. Angle from the vertical → vertical takes cos. Always identify the adjacent side first.

Displacement from perpendicular components

9702/23 M/J 2024 Q2(b)(iv)

An object is projected horizontally at a speed of 6.0 m s−16.0\ \text{m s}^{-1} from a slope, as shown in Fig. 2.1.

The slope is at an angle θ\theta to the horizontal. Air resistance is negligible.

The object lands on the slope a time of 0.71 s0.71\ \text{s} later and stops without rolling or bouncing.

(Earlier parts of the question find the horizontal distance travelled, 4.3 m4.3\ \text{m}, and the vertical distance travelled, 2.5 m2.5\ \text{m}.)

Determine the magnitude of the displacement of the object from its original position.

Fig. 2.1 from the question paper.

Fig. 2.1 from the question paper.

Show full working
  1. 1

    Displacement is a vector. Its two components — 4.3 m4.3\ \text{m} horizontally and 2.5 m2.5\ \text{m} vertically — are perpendicular, so the magnitude comes from Pythagoras, not from addition.

    This is the whole point of the question: adding 4.3 + 2.5 = 6.8 m treats the components as scalars and throws away their directions.

  2. 2

    Substitute into R=Rx2+Ry2R = \sqrt{R_x^2 + R_y^2}: s=4.32+2.52s = \sqrt{4.3^2 + 2.5^2}

  3. 3

    Evaluate each square first: 4.32=18.494.3^2 = 18.49 and 2.52=6.252.5^2 = 6.25, so s=18.49+6.25=24.74s = \sqrt{18.49 + 6.25} = \sqrt{24.74}

  4. 4

    Take the root and round: s=4.97 m≈5.0 ms = 4.97\ \text{m} \approx 5.0\ \text{m} (2 s.f. to match the data).

Answer

s≈5.0 ms \approx 5.0\ \text{m} (from 4.32+2.52=4.97 m\sqrt{4.3^2 + 2.5^2} = 4.97\ \text{m}; the mark scheme accepts 4.9 m4.9\ \text{m} or 5.0 m5.0\ \text{m}).

Whenever a question asks for displacement (or any vector) from two perpendicular pieces, Pythagoras is the reflex — never plain addition.

Your turn

  1. 19702/14 M/J 2025 Q4

    The diagram shows two fixed pins, Y and Z. A length of elastic is stretched between Y and Z and around pin X, which is attached to a trolley.

    X is at the centre of the elastic and the trolley is to be propelled in the direction P at right angles to YZ. The tension in the elastic is 4.0 N4.0\ \text{N}.

    What is the force accelerating the trolley in the direction P when the trolley is released?

    Options

    A   2.4 N2.4\ \text{N}
    B   3.2 N3.2\ \text{N}
    C   4.8 N4.8\ \text{N}
    D   6.4 N6.4\ \text{N}

    Fig. 1 from the question paper.

    Fig. 1 from the question paper.

    Stuck? Show hint

    First find the angle each 50 mm segment makes with P from the printed geometry: 30 mm along P, 50 mm of segment.

    Show solution
    1. 1

      Geometry first. Drop a perpendicular from X to the midpoint of YZ: it runs 30 mm30\ \text{mm} along direction P, and the segment itself is 50 mm50\ \text{mm} long. So for the angle θ\theta between a segment and P:

      cos⁡θ=3050=0.6⟹θ=53∘\cos\theta = \frac{30}{50} = 0.6 \quad\Longrightarrow\quad \theta = 53^\circ

      The angle is not given as a number — it has to be earned from the printed lengths before any resolving can happen.

    2. 2

      Resolve one tension along P (the adjacent component, so cos):

      Falong P=4.0×cos⁡53∘=4.0×0.6=2.4 NF_{\text{along P}} = 4.0 \times \cos 53^\circ = 4.0 \times 0.6 = 2.4\ \text{N}
    3. 3

      The components perpendicular to P from the two segments are equal and opposite — they cancel by symmetry. Only the components along P add, and there are two segments:
      R=2×2.4=4.8 NR = 2 \times 2.4 = 4.8\ \text{N} — option C.

      Forgetting the factor of 2 (both segments pull) gives 2.4 N, option A. Using sin instead of cos gives 4.0 × 0.8 = 3.2 N per segment, which leads to options B and D.

    Answer

    C — 4.8 N4.8\ \text{N} along P (2×4.0cos⁡53∘2 \times 4.0\cos 53^\circ, with the perpendicular components cancelling).

  2. 2

    A sledge is pulled by a force of 50 N50\ \text{N} along a rope held at 40∘40^\circ above the horizontal. (a) Calculate the horizontal and vertical components of the force. (b) The sledge slides along the ground: state which component pulls it forward and which tends to lift it.

    Show solution
    1. 1

      (a) The angle is measured from the horizontal, so the horizontal component is adjacent and takes cos:

      Fx=50cos⁡40∘=50×0.766=38.3≈38 NF_x = 50\cos 40^\circ = 50 \times 0.766 = 38.3 \approx 38\ \text{N}
    2. 2

      The vertical component is opposite and takes sin:

      Fy=50sin⁡40∘=50×0.643=32.1≈32 NF_y = 50\sin 40^\circ = 50 \times 0.643 = 32.1 \approx 32\ \text{N}
    3. 3

      (b) The horizontal component (38 N38\ \text{N}) acts along the ground and does the pulling forward; the vertical component (32 N32\ \text{N}) points upward and tends to lift the sledge, slightly reducing its contact force with the ground.

      (b) is the reason resolving is useful: along-the-ground and up-and-down effects can be analysed separately, because perpendicular components are independent.

    Answer

    (a) 38 N38\ \text{N} horizontal, 32 N32\ \text{N} vertical. (b) Horizontal pulls it forward; vertical tends to lift it.

  3. 3

    A walker's displacement consists of 12 m12\ \text{m} east followed by 5 m5\ \text{m} north. Find the magnitude and direction of the single displacement that has the same effect.

    Stuck? Show hint

    East and north are perpendicular — Pythagoras for the size, tan for the direction.

    Show solution
    1. 1

      The two legs are perpendicular, so the resultant has magnitude

      R=122+52=144+25=169=13 mR = \sqrt{12^2 + 5^2} = \sqrt{144 + 25} = \sqrt{169} = 13\ \text{m}
    2. 2

      Direction: measure the angle θ\theta from the easterly direction (the adjacent side):

      tan⁡θ=RyRx=512=0.4167⟹θ=22.6∘\tan\theta = \frac{R_y}{R_x} = \frac{5}{12} = 0.4167 \quad\Longrightarrow\quad \theta = 22.6^\circ
    3. 3

      So the single displacement is 13 m13\ \text{m} at 22.6∘22.6^\circ north of east.

      "North of east" names the reference axis — the angle is measured starting from east and rotating toward north. A direction without its reference is incomplete.

    Answer

    13 m13\ \text{m} at 22.6∘22.6^\circ north of east.

  4. 4

    Two forces act at a point: 10.0 N10.0\ \text{N} along the xx-direction, and 8.0 N8.0\ \text{N} at 60∘60^\circ to the xx-direction. Find the resultant force by resolving both forces into xx- and yy-components, adding the components, and recombining. Check your answer with the cosine rule.

    Stuck? Show hint

    The 10.0 N10.0\ \text{N} force has no yy-component. Resolve only the 8.0 N8.0\ \text{N} force.

    Show solution
    1. 1

      Components of the 10.0 N10.0\ \text{N} force: it lies along xx, so F1x=10.0 NF1y=0F_{1x} = 10.0\ \text{N} \qquad F_{1y} = 0

    2. 2

      xx-component of the 8.0 N8.0\ \text{N} force (angle measured from xx, so cos): F2x=8.0cos⁡60∘=8.0×0.500=4.0 NF_{2x} = 8.0\cos 60^\circ = 8.0 \times 0.500 = 4.0\ \text{N}

    3. 3

      yy-component of the 8.0 N8.0\ \text{N} force (sin): F2y=8.0sin⁡60∘=8.0×0.866=6.93 NF_{2y} = 8.0\sin 60^\circ = 8.0 \times 0.866 = 6.93\ \text{N}

    4. 4

      Add the components along each direction separately: Rx=10.0+4.0=14.0 NRy=0+6.93=6.93 NR_x = 10.0 + 4.0 = 14.0\ \text{N} \qquad R_y = 0 + 6.93 = 6.93\ \text{N}

      Components along the same direction add like ordinary numbers. Never add an x-component to a y-component.

    5. 5

      Recombine the magnitude with Pythagoras: R=14.02+6.932=196+48.0=244=15.6 NR = \sqrt{14.0^2 + 6.93^2} = \sqrt{196 + 48.0} = \sqrt{244} = 15.6\ \text{N}

    6. 6

      Direction from the xx-direction: tan⁡θ=RyRx=6.9314.0=0.495⟹θ=26∘\tan\theta = \frac{R_y}{R_x} = \frac{6.93}{14.0} = 0.495 \quad\Longrightarrow\quad \theta = 26^\circ

    7. 7

      Check with the cosine rule, A=10.0A = 10.0, B=8.0B = 8.0, angle 60∘60^\circ: R2=10.02+8.02+2(10.0)(8.0)cos⁡60∘=100+64+80=244R^2 = 10.0^2 + 8.0^2 + 2(10.0)(8.0)\cos 60^\circ = 100 + 64 + 80 = 244 so R=15.6 NR = 15.6\ \text{N} ✓.

      Both methods give the same answer. Components are easier when there are three or more vectors; the cosine rule is quicker for exactly two.

    Answer

    15.6 N15.6\ \text{N} at 26∘26^\circ to the xx-direction.

Common mistakes
  • The weight of a 70 kg70\ \text{kg} person is 70 N70\ \text{N}.

    W=mg=70×9.81≈690 NW = mg = 70 \times 9.81 \approx 690\ \text{N}.

    kg is a mass unit and N a force unit; weight needs the ×g conversion every time.

  • 1 cm2=10−2 m21\ \text{cm}^2 = 10^{-2}\ \text{m}^2.

    1 cm2=(10−2 m)2=10−4 m21\ \text{cm}^2 = (10^{-2}\ \text{m})^2 = 10^{-4}\ \text{m}^2.

    The index squares the power of ten along with the unit — the same applies to mm², cm³ and every prefixed unit carrying an exponent.

  • Precise data is accurate data.

    Precision is the scatter between repeats; accuracy is closeness of the mean to the true value — a systematic error produces tight, wrong data.

    The two words answer different questions: how well do repeats agree with each other, versus how close is the result to the truth.

  • Add the percentage uncertainties of a sum.

    Sums and differences add ABSOLUTE uncertainties; products and quotients add PERCENTAGE uncertainties.

    Using the wrong rule loses the uncertainty marks — check which operation combines the quantities before choosing.

  • The resultant of two forces is A+BA + B, so two 6 N6\ \text{N} forces at 60∘60^\circ give 12 N12\ \text{N}.

    Use the cosine rule: R2=62+62+2(6)(6)cos⁡60∘=108R^2 = 6^2 + 6^2 + 2(6)(6)\cos 60^\circ = 108, so R≈10 NR \approx 10\ \text{N}.

    Plain addition only works when the vectors point the same way (θ = 0); any other angle needs the cosine rule.

  • sin goes with the horizontal component.

    cos goes with the adjacent side — the component along the direction the angle is measured from. Check: at θ = 0 the whole vector lies along the axis, and cos 0 = 1.

    Which function goes where depends on which axis θ was measured from, not on "horizontal" or "vertical" as words — the θ = 0 check settles it every time.

In the exam
351 marks · 271 parts · 37 sittings · 2021–2025 · mean difficulty 1.79 · rank 9 of 11

On 9702 Papers 1+2 (2021–2025) this topic supplied 351 marks across 271 question parts in 37 sittings of Papers 1 and 2 — roughly 9 or 10 marks a sitting — and its techniques (base units, uncertainty rules, component resolution) come back inside later topics. Return to this note whenever a later topic assumes one of those skills.

Everything on one page

Fx=Fcos⁡θ,Fy=Fsin⁡θF_x = F\cos\theta, \qquad F_y = F\sin\theta

Components of a vector F at angle θ to the x-direction

R=Rx2+Ry2,tan⁡θ=RyRxR = \sqrt{R_x^2 + R_y^2}, \qquad \tan\theta = \frac{R_y}{R_x}

Recombining perpendicular components into a resultant

R2=A2+B2+2ABcos⁡θR^2 = A^2 + B^2 + 2AB\cos\theta

Resultant of two vectors with angle θ between them (cosine-rule form)

Δv⃗=v⃗−u⃗=v⃗+(−u⃗)\Delta\vec{v} = \vec{v} - \vec{u} = \vec{v} + (-\vec{u})

Change in a vector: final minus initial, i.e. add the reversed initial vector

p 10−12, n 10−9, μ 10−6, m 10−3, c 10−2, d 10−1, k 103, M 106, G 109, T 1012\text{p}\ 10^{-12},\ \text{n}\ 10^{-9},\ \mu\ 10^{-6},\ \text{m}\ 10^{-3},\ \text{c}\ 10^{-2},\ \text{d}\ 10^{-1},\ \text{k}\ 10^{3},\ \text{M}\ 10^{6},\ \text{G}\ 10^{9},\ \text{T}\ 10^{12}

Prefixes (recall): pico, nano, micro, milli, centi, deci, kilo, mega, giga, tera

mass (kg), length (m), time (s), current (A), temperature (K)\text{mass (kg), length (m), time (s), current (A), temperature (K)}

The five SI base quantities and units (recall)

y=a±b: Δy=Δa+Δby=ab or ab: Δyy=Δaa+Δbby=an: Δyy=nΔaay = a \pm b:\ \Delta y = \Delta a + \Delta b \qquad y = ab \text{ or } \tfrac{a}{b}:\ \tfrac{\Delta y}{y} = \tfrac{\Delta a}{a} + \tfrac{\Delta b}{b} \qquad y = a^n:\ \tfrac{\Delta y}{y} = n\tfrac{\Delta a}{a}

Combining uncertainties: sums/differences add absolute uncertainties; products/quotients add fractional (percentage) ones; a power n multiplies by n; exact constants add nothing

1 N=1 kg m s−2;1 J=1 N m=1 kg m2 s−2;1 W=1 J s−1=1 kg m2 s−3;1 Pa=1 N m−2=1 kg m−1 s−2;1 C=1 A s1\text{ N} = 1\ \text{kg m s}^{-2}; \quad 1\text{ J} = 1\ \text{N m} = 1\ \text{kg m}^2\text{ s}^{-2}; \quad 1\text{ W} = 1\ \text{J s}^{-1} = 1\ \text{kg m}^2\text{ s}^{-3}; \quad 1\text{ Pa} = 1\ \text{N m}^{-2} = 1\ \text{kg m}^{-1}\text{ s}^{-2}; \quad 1\text{ C} = 1\ \text{A s}

Derived units expressed in base units (each built from its defining equation)

Can you do all of these?

  • State that every physical quantity is a magnitude with a unit, and make order-of-magnitude estimates anchored to known reference values

  • Recall the five SI base quantities (kg, m, s, A, K) — charge, force and energy are NOT base quantities — and express derived units as products/quotients of base units

  • Convert between prefixed units from pico to tera, including squared/cubed prefixes and compound units

  • Check the homogeneity of an equation in base units, find the base units of a constant, and find an unknown power by matching indices

  • Distinguish systematic (including zero) errors from random errors, correct a zero error, and tell precision from accuracy

  • Combine absolute uncertainties for sums/differences and percentage uncertainties for products/quotients, multiplying by n for powers

  • Quote a derived value with its uncertainty rounded to 1 significant figure, the value's last figure matching; compare two results by checking whether their ranges overlap

  • Classify quantities as scalars or vectors, and add/subtract coplanar vectors head-to-tail or with the cosine rule; find a change in velocity as v − u

  • Resolve a vector into perpendicular components with cos/sin, add vectors component by component, and recombine with Pythagoras and tan